This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 22.2648 2461152.7648 11.10 10:11:49.49 +15:35:25.6
221.92028 51.27573 galactic Leo Second-epoch detections are separated by 0.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.11 Parthenope -1 0 1 11.4 0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 10:11:49.49 +15:35:25.6: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 10:11:49.49 +15:35:25.6: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 22.2648* 10 11 49.49 +15 35 25.6 11.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.7648,11.10,0.05,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 20260422.2648 11.10CV 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 04 22.2648 2461152.7648 12.68 09:50:02.07 +16:18:14.5
217.76312 46.74484 galactic Leo Second-epoch detections are separated by 0.5" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.103 Hera -1 2 2 12.9 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 09:50:02.07 +16:18:14.5: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 09:50:02.07 +16:18:14.5: 16.06 +/- 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 04 22.2648* 09 50 02.07 +16 18 14.5 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.7648,12.68,0.05,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 20260422.2648 12.68CV 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 04 22.2648 2461152.7648 13.20 09:33:23.67 +09:29:08.1
223.89834 40.17448 galactic Leo Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.67 Asia -1 1 1 13.4 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 09:33:23.67 +09:29:08.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 09:33:23.67 +09:29:08.1: 16.00 +/- 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 04 22.2648* 09 33 23.67 +09 29 08.1 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.7648,13.20,0.05,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 20260422.2648 13.20CV 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 04 22.2648 2461152.7648 13.55 10:04:38.25 +18:19:17.7
216.86587 50.72814 galactic Leo Second-epoch detections are separated by 0.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.161 Athor -1 1 2 14.0 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 10:04:38.25 +18:19:17.7: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 10:04:38.25 +18:19:17.7: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 22.2648* 10 04 38.25 +18 19 17.7 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,2461152.7648,13.55,0.05,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 20260422.2648 13.55CV 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
Mean magnitude and position on the discovery images:
2026 04 22.2648 2461152.7648 13.63 09:38:13.51 +16:39:11.8
215.77620 44.25514 galactic Leo Second-epoch detections are separated by 1.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.47 Aglaja -2 1 2 13.8 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 09:38:13.51 +16:39:11.8: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 09:38:13.51 +16:39:11.8: 16.10 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 22.2648* 09 38 13.51 +16 39 11.8 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,2461152.7648,13.63,0.05,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 20260422.2648 13.63CV 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 04 22.2648 2461152.7648 14.17 10:08:29.55 +10:13:02.3
228.76729 48.12059 galactic Leo Second-epoch detections are separated by 1.1" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.808 Merxia -1 2 2 14.5 0 -0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 10:08:29.55 +10:13:02.3: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 10:08:29.55 +10:13:02.3: 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 04 22.2648* 10 08 29.55 +10 13 02.3 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.7648,14.17,0.05,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 20260422.2648 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.2648 2461152.7648 14.98 10:12:37.87 +17:56:27.6
218.53453 52.36378 galactic Leo Second-epoch detections are separated by 1.8" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.909 Ulla -2 1 2 15.0 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 10:12:37.87 +17:56:27.6: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 10:12:37.87 +17:56:27.6: 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 04 22.2648* 10 12 37.87 +17 56 27.6 15.0 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,2461152.7648,14.98,0.05,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 20260422.2648 14.98CV 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 04 22.2648 2461152.7648 14.88 09:37:29.65 +16:28:03.2
215.92481 44.02318 galactic Leo Second-epoch detections are separated by 0.3" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.75 Eurydike -2 1 3 15.2 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 09:37:29.65 +16:28:03.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 09:37:29.65 +16:28:03.2: 16.16 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 22.2648* 09 37 29.65 +16 28 03.2 14.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.7648,14.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260422.2648 14.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 22.2648 2461152.7648 14.82 09:29:49.61 +14:07:43.6
217.87283 41.40773 galactic Leo Second-epoch detections are separated by 1.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.318 Magdalena -1 2 2 14.9 -0 0
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits at 09:29:49.61 +14:07:43.6: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits at 09:29:49.61 +14:07:43.6: 16.14 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 22.2648* 09 29 49.61 +14 07 43.6 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461152.7648,14.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260422.2648 14.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
First image: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Last image: 2461152.76511059 22.04.2026 06:21:35.555 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 7782
Objects passed selection criteria: 7776
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 7058.25
Average stars matched: 6885.75 (97.5561 %)
Memory usage VmPeak: 113372 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 22 01:24:01 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: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
First image: 2461058.86919819 18.01.2026 08:51:28.724 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Last image: 2461152.76511059 22.04.2026 06:21:35.555 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 13 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 43039
Objects passed selection criteria: 42923
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 40453.8
Average stars matched: 39216 (96.9403 %)
Memory usage VmPeak: 142876 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 22 01:25:32 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461152.76442471
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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits exists and is non-empty
Saving wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits to local_wcs_cache/
'wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits'
wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits exists and is non-empty
Saving wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits to local_wcs_cache/
'wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits' -> 'local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:34.262 +13:59:45.34 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:36.703 +13:55:44.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:36.703 +13:55:44.07
Angular distance between the image centers 0.0677 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:36.624 +13:56:13.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:36.624 +13:56:13.01
Angular distance between the image centers 0.0597 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 09:46:36.703 +13:55:44.07
Second-epoch second image center 09:46:36.624 +13:56:13.01
Angular distance between the image centers 0.00805 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.GBLWZSTo3p
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits &> /tmp/tmp.D8XeYcZyPE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits &> /tmp/tmp.BAgd5dgWmG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits &> /tmp/tmp.uUmyeUTQNV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
Found non-empty wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
The reference image (wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat) found
'wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat' -> 'wcsmag.cat'
Read 7958 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3852 to 154.9366 deg, Dec +8.6225 to +19.2659 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 138.3852 to 154.9366 deg, Dec 8.6225 to 19.2659 deg
Loaded 4773 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): 3901 out of 4125 total matches.
Matched with Tycho-2 4125 out of 7958 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893593
a=0.000000 b=1.000000 c=22.893593
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7958 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3852 to 154.9366 deg, Dec +8.6225 to +19.2659 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 138.3852 to 154.9366 deg, Dec 8.6225 to 19.2659 deg
Loaded 4773 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): 3901 out of 4125 total matches.
Matched with Tycho-2 4125 out of 7958 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits (aperture=6.2)
Read 8039 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3853 to 154.9366 deg, Dec +8.6284 to +19.2860 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 138.3853 to 154.9366 deg, Dec 8.6284 to 19.2860 deg
Loaded 4774 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3915 out of 4145 total matches.
Matched with Tycho-2 4145 out of 8039 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
2.1 pix Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
2.2 pix fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
2.2 pix fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
2.1 pix wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
2.1 pix wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Limiting magnitude estimates:
15.4 mag. Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
15.4 mag. Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
15.0 mag. fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
15.1 mag. fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GBLWZSTo3p (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=534, passed=7958
Got 7958 stars (including 7414 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 7958 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7692 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 7692 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.D8XeYcZyPE (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> 'wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=535, passed=8039
Got 8039 stars (including 7496 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 8039 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 7745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits -region wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BAgd5dgWmG (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=6213
Got 6213 stars (including 5806 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat
util/solve_plate_with_UCAC5 got 6213 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
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.5)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 6030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.5)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 6029 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 6029 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits -region wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uUmyeUTQNV (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=397, passed=6219
Got 6219 stars (including 5811 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
util/solve_plate_with_UCAC5 got 6219 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
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 6017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 6016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 911 matched stars entering correct_measured_positions(), 6016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits -region wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits'
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits'
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20528.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20461_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 20461_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:15:09.13 +13:50:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20528_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 20528_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
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 ####
10:11:49.49 +15:35:25.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
SExtractor catalog cache: saved Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits exists and is non-empty
wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits (1st reference image)
verification OK: wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:34.262 +13:59:45.34 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits (1st new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:36.703 +13:55:44.07 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:36.703 +13:55:44.07
Angular distance between the image centers 0.0677 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits (2nd new image)
verification OK: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Image size: 941.5'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:46:36.624 +13:56:13.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:46:34.262 +13:59:45.34
Second-epoch image center 09:46:36.624 +13:56:13.01
Angular distance between the image centers 0.0597 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 09:46:36.703 +13:55:44.07
Second-epoch second image center 09:46:36.624 +13:56:13.01
Angular distance between the image centers 0.00805 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.XJAGEgxtu6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits &> /tmp/tmp.kzeXeN6NXS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits &> /tmp/tmp.9nSFgrPCWG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits &> /tmp/tmp.EKYrK6aSmC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
Found non-empty wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits and wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
The reference image (wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits) and catalog (wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat) found
'wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat' -> 'wcsmag.cat'
Read 43775 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3793 to 154.9626 deg, Dec +8.6120 to +19.2857 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 138.3793 to 154.9626 deg, Dec 8.6120 to 19.2857 deg
Loaded 4796 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): 3707 out of 4153 total matches.
Matched with Tycho-2 4153 out of 43775 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.782622
a=0.000000 b=1.000000 c=22.782622
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 43775 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3793 to 154.9626 deg, Dec +8.6120 to +19.2857 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 138.3793 to 154.9626 deg, Dec 8.6120 to 19.2857 deg
Loaded 4796 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): 3707 out of 4153 total matches.
Matched with Tycho-2 4153 out of 43775 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits (aperture=4.9)
Read 43730 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 138.3631 to 154.9630 deg, Dec +8.6125 to +19.2926 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 138.3631 to 154.9630 deg, Dec 8.6125 to 19.2926 deg
Loaded 4803 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): 3714 out of 4157 total matches.
Matched with Tycho-2 4157 out of 43730 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits -> calib.txt_param_ref_wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
2.0 pix Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
2.0 pix fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
2.0 pix fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
2.0 pix wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
2.0 pix wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Limiting magnitude estimates:
15.5 mag. Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
15.5 mag. Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
15.2 mag. fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
15.2 mag. fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XJAGEgxtu6 (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.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_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1969, passed=43753
Got 43753 stars (including 41699 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 43753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 42351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 42344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 42344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-51-28_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kzeXeN6NXS (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits' -> 'wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
Checking if the catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat corresponding to the image wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.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_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits
WCS catalog name: wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1988, passed=43712
Got 43712 stars (including 41658 good ones) from the SExtractor catalog wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 43712 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 42220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 42218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 42219 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits -region wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-04-Q1b1x1_2026-01-18_02-52-09_20.00sec_-14.90C_LIGHT_0401.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9nSFgrPCWG (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1345, passed=37523
Got 37523 stars (including 36099 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat
util/solve_plate_with_UCAC5 got 37523 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
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 36409 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
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 36410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 36410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits -region wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EKYrK6aSmC (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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS_IMAGE_NAME=wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS-calibrated image found: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Checking if the catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat corresponding to the image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
WCS catalog name: wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1372, passed=37911
Got 37911 stars (including 36474 good ones) from the SExtractor catalog wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat
util/solve_plate_with_UCAC5 got 37911 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
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 36730 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
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 36732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 36731 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits -region wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-20-36_20.00sec_-4.90C_LIGHTs_0133.fits
Saving fully-calibrated image wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.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_2026-04-22_CI_Leo-04-Q1b1x1_012233_TTUQ1b1x1_1820469_NKk5JrBP/wcs_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134.fits
Preparing the HTML report for the field Leo-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out54114.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54144.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 52934_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 52934_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:40:24.96 +15:23:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52944_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 52944_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:39:26.48 +14:13:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52946_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 52946_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:16:53.67 +10:56:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.123 593351419865063552 139.22351036169 +10.94615337050 13.6860 13.1995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52948_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 52948_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:24:41.44 +11:37:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53015_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53015_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:11:49.50 +15:35:25.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53122_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53122_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:42:58.03 +17:02:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53178_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 53178_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 53199_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53199_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:51:35.87 +17:28:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53221_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53221_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:30:25.82 +12:57:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53266_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53266_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:39:00.85 +14:25:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53325_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 53325_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 53337_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53337_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:48:01.94 +18:05:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53354_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53354_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:59:33.26 +09:20:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53356_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53356_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:31:51.15 +17:15:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53363_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53363_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:31:05.06 +11:30:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53386_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 53386_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 53410_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53410_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:04:22.54 +13:37:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53417_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53417_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:17:20.74 +16:32:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53432_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53432_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:00:27.47 +10:54:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53452_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 53452_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 53460_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53460_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:29:04.19 +17:44:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53480_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53480_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:32:04.40 +11:19:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53513_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53513_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 53531_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53531_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:52:12.33 +16:27:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53574_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53574_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:39:26.87 +16:46:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.848 620504679851630208 144.86180778568 +16.77573030203 14.0031 13.5045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53578_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53578_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:29:04.53 +17:51:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53579_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53579_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:53:14.96 +09:36:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53596_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 53596_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 53599_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53599_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:05:35.48 +15:44:27.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53623_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53623_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:44:02.22 +17:34:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53635_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53635_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:08:30.43 +16:38:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.145 622035994606664192 152.12734061324 +16.63447537960 13.8566 12.8116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53647_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53647_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:15:16.54 +09:45:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53688_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53688_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:30:38.67 +17:04:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53718_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53718_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:53:08.44 +09:35:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.801 3878948178070510336 148.28488034095 +09.59444167786 14.3730 13.8142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53726_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53726_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:35:13.89 +10:16:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53755_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53755_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:33:33.89 +18:43:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 4.637 633212049266442240 143.39054133623 +18.73021086765 14.3545 13.5474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53856_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53856_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:10:18.58 +11:17:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53860_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53860_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:33:10.81 +15:43:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53896_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53896_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:40:35.35 +15:02:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53923_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53923_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:52:58.32 +12:55:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.567 615043753488782336 148.24309941338 +12.92263105905 14.4928 13.7477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53931_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53931_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:39:23.03 +13:17:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53934_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53934_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:43:23.28 +12:37:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53976_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 53976_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:23:55.71 +12:47:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54005_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54005_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:34:34.26 +16:56:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54007_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54007_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:39:15.71 +12:26:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54009_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54009_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:15:56.84 +09:04:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54023_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 54023_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 54026_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54026_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:14:36.52 +08:39:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.165 3875734202503013376 153.65188396298 +08.65610745135 14.7840 14.2145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54071_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54071_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:21:59.64 +15:56:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 1.104 630944512692692096 140.49850573814 +15.94438791905 14.9237 14.3165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54090_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54090_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:14:32.86 +14:22:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.816 3887950532602015616 153.63674692979 +14.38201048757 14.8175 13.9860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54107_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54107_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:09:21.92 +14:47:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 2.963 3888142259941790336 152.34057768541 +14.78642665167 15.0488 14.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54108_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54108_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 10:10:47.88 +09:14:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.303 3876765230884570368 152.69959528873 +09.24028928258 15.2853 14.4818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54114_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54114_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:46:27.25 +17:32:00.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)
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Considering the candidate 54129_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54129_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
**** FOUND 09:23:58.95 +18:18:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54130_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 54130_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 54144_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
Preparing report for the candidate 54144_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
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Considering the candidate 54148_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134
The candidate 54148_fd_Leo-04-Q1b1x1_2026-04-22_01-21-35_20.00sec_-4.90C_LIGHTs_0134 did not pass the final checks
