This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N
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 06.4290* 09 31 05.63 +15 20 19.6 7.5 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,2461319.9290,7.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 7.53CV 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 06.4290 2461319.9290 10.55 09:16:30.81 +11:10:11.4
219.58290 37.21835 galactic Cnc Second-epoch detections are separated by 1.2" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.6 Hebe 0 0 0 10.8 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:16:30.81 +11:10:11.4: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:16:30.81 +11:10:11.4: 15.64 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461319.9290,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 10.55CV 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 06.4290* 09 30 56.16 +15 21 12.7 8.0 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,2461319.9290,7.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 7.96CV 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 06.4290* 09 31 05.88 +15 20 17.5 8.0 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,2461319.9290,7.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 7.99CV 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 06.4290 2461319.9290 11.47 10:01:59.90 +10:11:28.4
227.64633 46.71394 galactic Leo Second-epoch detections are separated by 1.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.10 Hygiea -0 -0 0 11.8 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:01:59.90 +10:11:28.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:01:59.90 +10:11:28.4: 15.97 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 06.4290* 10 01 59.90 +10 11 28.4 11.5 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,2461319.9290,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 11.47CV 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 06.4290 2461319.9290 11.96 10:08:59.06 +10:49:58.8
228.04834 48.52700 galactic Leo Second-epoch detections are separated by 3.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.16 Psyche 0 -0 0 12.2 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:59.06 +10:49:58.8: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:59.06 +10:49:58.8: 15.90 +/- 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 06.4290* 10 08 59.06 +10 49 58.8 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,2461319.9290,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 11.96CV 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 06.4290 2461319.9290 12.47 09:54:03.84 +18:19:10.1
215.50672 48.37866 galactic Leo Second-epoch detections are separated by 0.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.196 Philomela -0 -0 0 12.9 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:54:03.84 +18:19:10.1: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:54:03.84 +18:19:10.1: 16.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 06.4290* 09 54 03.84 +18 19 10.1 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,2461319.9290,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 12.47CV 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 06.4290 2461319.9290 13.00 09:37:58.71 +12:48:22.5
220.60143 42.66084 galactic Leo Second-epoch detections are separated by 2.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.747 Winchester -1 1 1 13.3 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:37:58.71 +12:48:22.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:37:58.71 +12:48:22.5: 16.07 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 06.4290* 09 37 58.71 +12 48 22.5 13.0 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,2461319.9290,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 13.00CV 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 06.4290 2461319.9290 13.54 09:40:08.60 +18:11:39.9
213.98614 45.23919 galactic Leo Second-epoch detections are separated by 1.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.245 Vera 1 -0 1 13.9 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:40:08.60 +18:11:39.9: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:40:08.60 +18:11:39.9: 16.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 06.4290* 09 40 08.60 +18 11 39.9 13.5 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,2461319.9290,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 06.4290 2461319.9290 13.59 09:26:40.15 +11:50:41.4
220.18055 39.75336 galactic Leo Second-epoch detections are separated by 1.3" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.584 Semiramis -0 1 1 13.8 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:26:40.15 +11:50:41.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:26:40.15 +11:50:41.4: 15.98 +/- 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 06.4290* 09 26 40.15 +11 50 41.4 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,2461319.9290,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 06.4290 2461319.9290 13.65 09:50:27.94 +15:12:21.8
219.29228 46.41084 galactic Leo Second-epoch detections are separated by 1.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.487 Venetia 1 1 1 13.9 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:50:27.94 +15:12:21.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:50:27.94 +15:12:21.8: 16.11 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 06.4290* 09 50 27.94 +15 12 21.8 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461319.9290,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 06.4290 2461319.9290 11.72 09:33:51.66 +14:01:07.0
218.54168 42.25673 galactic Leo Second-epoch detections are separated by 2.1" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.52 Europa -1 0 1 12.3 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:33:51.66 +14:01:07.0: 13.82 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:33:51.66 +14:01:07.0: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
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 06.4290* 09 33 51.66 +14 01 07.0 11.7 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,2461319.9290,11.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261006.4290 11.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
First image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461319.92927727 06.10.2026 10:17:59.556 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
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: 7 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): 6931
Objects passed selection criteria: 6917
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 5317
Average stars matched: 5212 (98.0252 %)
Memory usage VmPeak: 233544 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 Wed Oct 7 02:16:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
First image: 2461119.68287475 20.03.2026 04:23:10.378 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Last image: 2461319.92927727 06.10.2026 10:17:59.556 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.11
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 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): 37750
Objects passed selection criteria: 37659
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 29061
Average stars matched: 27704.5 (95.3322 %)
Memory usage VmPeak: 261632 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 Wed Oct 7 02:17:59 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.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: 2461319.92869546
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:46:31.656 +14:00:33.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Image size: 944.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:26.712 +14:01:13.43 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 09:46:26.712 +14:01:13.43
Angular distance between the image centers 0.0229 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Image size: 944.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:28.547 +14:00:33.74 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 09:46:28.547 +14:00:33.74
Angular distance between the image centers 0.0126 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 09:46:26.712 +14:01:13.43
Second-epoch second image center 09:46:28.547 +14:00:33.74
Angular distance between the image centers 0.01329 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.keyStCbnau
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.yBWpE3ycqk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits &> /tmp/tmp.uxiqOZO9Zk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits &> /tmp/tmp.amhiM12Xx7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat' -> 'wcsmag.cat'
Read 7795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4767 to 154.9673 deg, Dec +8.5555 to +19.3045 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4767 to 154.9673 deg, Dec 8.5555 to 19.3045 deg
Loaded 4795 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3891 out of 4080 total matches.
Matched with Tycho-2 4080 out of 7795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.915200
a=0.000000 b=1.000000 c=22.915200
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4767 to 154.9673 deg, Dec +8.5555 to +19.3045 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4767 to 154.9673 deg, Dec 8.5555 to 19.3045 deg
Loaded 4795 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3891 out of 4080 total matches.
Matched with Tycho-2 4080 out of 7795 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (aperture=6.6)
Read 7228 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4289 to 155.2668 deg, Dec +8.1760 to +19.5844 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4289 to 155.2668 deg, Dec 8.1760 to 19.5844 deg
Loaded 5216 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3897 out of 4082 total matches.
Matched with Tycho-2 4082 out of 7228 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.1 pix Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Limiting magnitude estimates:
15.5 mag. Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.5 mag. Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
14.0 mag. fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
14.0 mag. fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.keyStCbnau (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=485, bad_region=0, passed=7795
Got 7795 stars (including 7304 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
util/solve_plate_with_UCAC5 got 7795 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4624 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 4604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 7795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4624 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 7795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 7795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4604 stars left (next iteration limit 5064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=4604 sigma_overall_arcsec=0.389 sigma_q1_arcsec=0.333 sigma_q2_arcsec=0.439 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.381 n_q1=1374 n_q2=1044 n_q3=1180 n_q4=1006 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.yBWpE3ycqk (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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, bad_region=0, passed=7228
Got 7228 stars (including 6724 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4626 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 4607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 7228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 4626 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 7228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4607 matched stars entering correct_measured_positions(), 7228 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4607 stars left (next iteration limit 5067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=4607 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.285 n_q1=1021 n_q2=1212 n_q3=1021 n_q4=1353 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.uxiqOZO9Zk (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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=246, bad_region=0, passed=3183
Got 3183 stars (including 2933 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat
util/solve_plate_with_UCAC5 got 3183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.4'
Seting catalog search parameters based on the expected field of view 944.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013117 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010493 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 2712 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2700 matched stars entering correct_measured_positions(), 2700 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2700 matched stars entering correct_measured_positions(), 3181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 2712 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2701 matched stars entering correct_measured_positions(), 3181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 2701 matched stars entering correct_measured_positions(), 3181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 2701 stars left (next iteration limit 2970)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2701 robust_rms=11.017 arcsec worst_region_rms=21.564 arcsec outer_annulus_rms=21.564 arcsec
SIP_REFIT: SIP order 3 trial: matched=2701 robust_rms=0.648 arcsec worst_region_rms=0.815 arcsec outer_annulus_rms=0.815 arcsec
SIP_REFIT: SIP order 5 trial: matched=2701 robust_rms=0.386 arcsec worst_region_rms=0.454 arcsec outer_annulus_rms=0.424 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2701 robust_rms_before=1.415 arcsec robust_rms_before_corrected=0.385 arcsec robust_rms_after=0.386 arcsec worst_region_rms_before=0.487 worst_region_rms_after=0.454 outer_annulus_rms_before=1.565 outer_annulus_rms_after=0.424
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.487 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits worst_region_rms_kept=0.487 arcsec robust_rms_kept=0.385 arcsec matched=2701
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits N_match=2701 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.433 sigma_q3_arcsec=0.333 sigma_q4_arcsec=0.375 n_q1=879 n_q2=485 n_q3=757 n_q4=580 worst_quadrant_to_overall_ratio=1.179
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.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.amhiM12Xx7 (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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=240, bad_region=0, passed=3225
Got 3225 stars (including 2982 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat
util/solve_plate_with_UCAC5 got 3225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.4'
Seting catalog search parameters based on the expected field of view 944.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013117 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010493 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 2748 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2735 matched stars entering correct_measured_positions(), 2735 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2735 matched stars entering correct_measured_positions(), 3223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 2747 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2737 matched stars entering correct_measured_positions(), 3223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 2737 matched stars entering correct_measured_positions(), 3223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 2737 stars left (next iteration limit 3008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2737 robust_rms=11.077 arcsec worst_region_rms=21.128 arcsec outer_annulus_rms=21.128 arcsec
SIP_REFIT: SIP order 3 trial: matched=2737 robust_rms=0.613 arcsec worst_region_rms=0.819 arcsec outer_annulus_rms=0.788 arcsec
SIP_REFIT: SIP order 5 trial: matched=2737 robust_rms=0.358 arcsec worst_region_rms=0.459 arcsec outer_annulus_rms=0.409 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2737 robust_rms_before=1.381 arcsec robust_rms_before_corrected=0.384 arcsec robust_rms_after=0.358 arcsec worst_region_rms_before=0.454 worst_region_rms_after=0.459 outer_annulus_rms_before=1.478 outer_annulus_rms_after=0.409
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.454 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits worst_region_rms_kept=0.454 arcsec robust_rms_kept=0.384 arcsec matched=2737
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits N_match=2737 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.365 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.345 sigma_q4_arcsec=0.357 n_q1=903 n_q2=497 n_q3=757 n_q4=580 worst_quadrant_to_overall_ratio=1.036
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
Saving the final (post-refit) wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
Saving the final (post-refit) wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits'
Saving the final (post-refit) wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits sigma_overall=0.389 worst_q_ratio=1.128
ref2=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits sigma_overall=0.309 worst_q_ratio=1.071
new1=fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits sigma_overall=0.368 worst_q_ratio=1.179
new2=fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits sigma_overall=0.360 worst_q_ratio=1.036
reference average sigma_overall=0.349 worst_q_ratio=1.0995
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155_astrometric_residuals.png (4604 matched stars from wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138_astrometric_residuals.png (4607 matched stars from wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464_astrometric_residuals.png (2701 matched stars from wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465_astrometric_residuals.png (2737 matched stars from wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits'
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:16:30.81 +11:10:11.4: 15.57 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:16:30.81 +11:10:11.4: 15.64 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20374.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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20363_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 20363_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20367_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 20367_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 09:35:55.49 +14:22:53.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20371_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 20371_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20374_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 20374_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20381_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 20381_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (30.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20383_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 20383_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (32.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20386_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 20386_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:16:30.81 +11:10:11.4
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-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits exists and is non-empty
wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:46:31.656 +14:00:33.25 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Image size: 944.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:26.712 +14:01:13.43 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 09:46:26.712 +14:01:13.43
Angular distance between the image centers 0.0229 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Image size: 944.4'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:28.547 +14:00:33.74 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 09:46:28.547 +14:00:33.74
Angular distance between the image centers 0.0126 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 09:46:26.712 +14:01:13.43
Second-epoch second image center 09:46:28.547 +14:00:33.74
Angular distance between the image centers 0.01329 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits &> /tmp/tmp.YZKzOQrfir
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits &> /tmp/tmp.5ea1TiNPBZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits &> /tmp/tmp.AJtXregjWN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits &> /tmp/tmp.3i3EHG7ulu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Found non-empty wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits and wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
The reference image (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat) found
'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat' -> 'wcsmag.cat'
Read 41224 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4693 to 154.9673 deg, Dec +8.5466 to +19.3048 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4693 to 154.9673 deg, Dec 8.5466 to 19.3048 deg
Loaded 4807 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3691 out of 4110 total matches.
Matched with Tycho-2 4110 out of 41224 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.790900
a=0.000000 b=1.000000 c=22.790900
From vast_summary.log: estimated ref. image limiting mag.: -7.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 41224 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.4693 to 154.9673 deg, Dec +8.5466 to +19.3048 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.4693 to 154.9673 deg, Dec 8.5466 to 19.3048 deg
Loaded 4807 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3691 out of 4110 total matches.
Matched with Tycho-2 4110 out of 41224 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (aperture=5.1)
Read 42226 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3847 to 155.2957 deg, Dec +8.1204 to +19.5912 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 138.3847 to 155.2957 deg, Dec 8.1204 to 19.5912 deg
Loaded 5273 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3733 out of 4126 total matches.
Matched with Tycho-2 4126 out of 42226 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
2.0 pix Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
2.6 pix fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Limiting magnitude estimates:
15.7 mag. Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
15.7 mag. Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
14.2 mag. fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
14.2 mag. fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.4 (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.YZKzOQrfir (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits' -> 'wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1984, bad_region=0, passed=41202
Got 41202 stars (including 39163 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat
util/solve_plate_with_UCAC5 got 41202 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4609 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 4594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 41202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4609 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 41202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4593 matched stars entering correct_measured_positions(), 41202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4593 stars left (next iteration limit 5052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits N_match=4593 sigma_overall_arcsec=0.379 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.435 sigma_q3_arcsec=0.383 sigma_q4_arcsec=0.373 n_q1=1357 n_q2=1062 n_q3=1139 n_q4=1035 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits -region wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.5ea1TiNPBZ (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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits' -> 'wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1796, bad_region=34, passed=42210
Got 42210 stars (including 40321 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 42210 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 4604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 42210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 4617 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 42210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4604 matched stars entering correct_measured_positions(), 42210 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4604 stars left (next iteration limit 5064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits N_match=4604 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.314 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.270 n_q1=1022 n_q2=1221 n_q3=1021 n_q4=1340 worst_quadrant_to_overall_ratio=1.057
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits -region wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.AJtXregjWN (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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=8, blended=602, bad_region=18, passed=16825
Got 16825 stars (including 16171 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat
util/solve_plate_with_UCAC5 got 16825 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.4'
Seting catalog search parameters based on the expected field of view 944.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013117 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010493 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4636 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 4617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 16825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4635 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 16825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4617 matched stars entering correct_measured_positions(), 16825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4617 stars left (next iteration limit 5078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.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=4617 robust_rms=10.550 arcsec worst_region_rms=22.016 arcsec outer_annulus_rms=22.016 arcsec
SIP_REFIT: SIP order 3 trial: matched=4617 robust_rms=0.647 arcsec worst_region_rms=0.780 arcsec outer_annulus_rms=0.780 arcsec
SIP_REFIT: SIP order 5 trial: matched=4617 robust_rms=0.426 arcsec worst_region_rms=0.514 arcsec outer_annulus_rms=0.466 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4617 robust_rms_before=1.429 arcsec robust_rms_before_corrected=0.388 arcsec robust_rms_after=0.426 arcsec worst_region_rms_before=0.470 worst_region_rms_after=0.514 outer_annulus_rms_before=1.589 outer_annulus_rms_after=0.466
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.470 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits worst_region_rms_kept=0.470 arcsec robust_rms_kept=0.388 arcsec matched=4617
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits N_match=4617 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.455 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.367 n_q1=1466 n_q2=810 n_q3=1383 n_q4=958 worst_quadrant_to_overall_ratio=1.217
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.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.3i3EHG7ulu (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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=527, bad_region=21, passed=16984
Got 16984 stars (including 16408 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat
util/solve_plate_with_UCAC5 got 16984 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.4'
Seting catalog search parameters based on the expected field of view 944.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013117 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010493 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4642 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4620 matched stars entering correct_measured_positions(), 4621 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4620 matched stars entering correct_measured_positions(), 16984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4642 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4622 matched stars entering correct_measured_positions(), 16984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4622 matched stars entering correct_measured_positions(), 16984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4622 stars left (next iteration limit 5082)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.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=4622 robust_rms=10.489 arcsec worst_region_rms=22.079 arcsec outer_annulus_rms=22.079 arcsec
SIP_REFIT: SIP order 3 trial: matched=4622 robust_rms=0.612 arcsec worst_region_rms=0.831 arcsec outer_annulus_rms=0.770 arcsec
SIP_REFIT: SIP order 5 trial: matched=4622 robust_rms=0.402 arcsec worst_region_rms=0.503 arcsec outer_annulus_rms=0.449 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4622 robust_rms_before=1.382 arcsec robust_rms_before_corrected=0.374 arcsec robust_rms_after=0.402 arcsec worst_region_rms_before=0.438 worst_region_rms_after=0.503 outer_annulus_rms_before=1.481 outer_annulus_rms_after=0.449
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.438 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits worst_region_rms_kept=0.438 arcsec robust_rms_kept=0.374 arcsec matched=4622
WCS_QUALITY_DIAG: file=fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits N_match=4622 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.345 sigma_q4_arcsec=0.366 n_q1=1469 n_q2=819 n_q3=1378 n_q4=956 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits -region wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-09_20.00sec_-0.00C_LIGHTs_0464.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.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_2026-10-06_CI_Leo-04-Q1b1x1_054020_TTUQ1b1x1_3200222_TfZf5y8N/wcs_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465.fits
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:18:27.77 +18:45:04.3: 13.61 +/- 0.06 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:08:59.06 +10:49:58.8: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:01:59.90 +10:11:28.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:54:03.84 +18:19:10.1: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:18:27.77 +18:45:04.3: 13.57 +/- 0.05 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:54:03.84 +18:19:10.1: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:01:59.90 +10:11:28.4: 15.97 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:08:59.06 +10:49:58.8: 15.90 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.59 +/- 0.04
Forced photometry filter REJECTED candidate at 09:18:27.77 +18:45:04.3: ref_mag=13.59 +/- 0.04 new_mean_mag=13.6701 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:37:58.71 +12:48:22.5: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:17:25.63 +16:32:43.9: 13.11 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:49:44.78 +11:07:02.7: 12.80 +/- 0.02 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:37:58.71 +12:48:22.5: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:17:25.63 +16:32:43.9: 13.42 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:49:44.78 +11:07:02.7: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry reference-image weighted average: 12.80 +/- 0.02
Forced photometry filter REJECTED candidate at 09:17:25.63 +16:32:43.9: ref_mag=13.24 +/- 0.02 new_mean_mag=13.3955 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:49:44.78 +11:07:02.7: ref_mag=12.80 +/- 0.02 new_mean_mag=12.7867 delta=0.01 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 10:01:25.27 +15:40:20.7: 13.06 +/- 0.03 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:40:08.60 +18:11:39.9: 16.10 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 10:01:25.27 +15:40:20.7: 12.97 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry filter REJECTED candidate at 10:01:25.27 +15:40:20.7: ref_mag=13.01 +/- 0.02 new_mean_mag=13.0621 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:40:08.60 +18:11:39.9: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:26:40.15 +11:50:41.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:50:27.94 +15:12:21.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:50:27.94 +15:12:21.8: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:26:40.15 +11:50:41.4: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-03-19_23-23-10_20.00sec_-15.00C_LIGHT_0155.fits at 09:33:51.66 +14:01:07.0: 13.82 +/- 0.04 detection
Forced photometry on wcs_Leo-04-Q1b1x1_2026-04-16_00-03-54_20.00sec_-4.90C_LIGHTs_0138.fits at 09:33:51.66 +14:01:07.0: 13.90 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.86 +/- 0.03
Forced photometry filter KEPT candidate at 09:33:51.66 +14:01:07.0: ref_mag=13.86 +/- 0.03 new_mean_mag=11.7040 delta=2.15 (need > 0.90)
Adding exclusion_list_local.txt__out21641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55143.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 8s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54788_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54788_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54790_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54790_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 09:15:09.14 +10:52:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54794_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 54794_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54795_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 54795_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54802_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54802_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 09:16:30.80 +11:10:11.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54837_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 54837_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54841_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54841_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 09:40:58.96 +09:52:39.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54854_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54854_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 10:08:08.80 +11:58:15.8 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54857_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 54857_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54859_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 54859_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54869_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54869_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 09:51:35.87 +17:28:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54877_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54877_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
**** FOUND 09:17:23.91 +13:03:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54920_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54920_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54930_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54930_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54943_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54943_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54958_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
Preparing report for the candidate 54958_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54980_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54980_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54988_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 54988_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55013_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 55013_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55042_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465
The candidate 55042_fd_Leo-04-Q1b1x1_2026-10-06_05-17-59_20.00sec_-0.00C_LIGHTs_0465 did not pass the final checks
