This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt
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 23.2916 2461153.7916 11.80 11:02:00.05 +04:59:17.8
248.38984 55.80106 galactic Leo Second-epoch detections are separated by 0.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.19 Fortuna -0 0 0 12.0 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:02:00.05 +04:59:17.8: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:02:00.05 +04:59:17.8: 15.88 +/- 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 23.2916* 11 02 00.05 +04 59 17.8 11.8 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,2461153.7916,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2916 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.2916 2461153.7916 11.85 11:25:38.98 +06:01:43.2
255.03497 60.65334 galactic Leo Second-epoch detections are separated by 0.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.65 Cybele -0 0 0 12.1 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:25:38.98 +06:01:43.2: 15.75 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:25:38.98 +06:01:43.2: 15.80 +/- 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 23.2916* 11 25 38.98 +06 01 43.2 11.8 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,2461153.7916,11.85,0.05,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 20260423.2916 11.85CV 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 23.2916 2461153.7916 12.55 11:09:51.45 +01:41:23.8
254.89645 54.79433 galactic Leo Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.120 Lachesis -1 1 1 12.7 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:09:51.45 +01:41:23.8: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:09:51.45 +01:41:23.8: 15.91 +/- 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 23.2916* 11 09 51.45 +01 41 23.8 12.6 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,2461153.7916,12.55,0.05,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 20260423.2916 12.55CV 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 23.2916 2461153.7916 12.67 10:48:39.59 +04:01:10.6
245.77879 52.69141 galactic Sex Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.270 Anahita 0 1 1 13.0 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 10:48:39.59 +04:01:10.6: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 10:48:39.59 +04:01:10.6: 15.80 +/- 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 23.2916* 10 48 39.59 +04 01 10.6 12.7 U Sex 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,2461153.7916,12.67,0.05,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 20260423.2916 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.2916 2461153.7916 13.23 11:14:05.50 +05:31:36.9
251.56378 58.32624 galactic Leo Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.453 Tea -0 0 1 13.4 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:14:05.50 +05:31:36.9: 16.08 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:14:05.50 +05:31:36.9: 16.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 23.2916* 11 14 05.50 +05 31 36.9 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,2461153.7916,13.23,0.05,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 20260423.2916 13.23CV 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 23.2916 2461153.7916 13.33 11:38:36.08 +04:32:10.8
262.17247 61.50219 galactic Vir Second-epoch detections are separated by 0.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.207 Hedda 0 -0 0 13.6 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:38:36.08 +04:32:10.8: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:38:36.08 +04:32:10.8: 15.69 +/- 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 23.2916* 11 38 36.08 +04 32 10.8 13.3 U Vir 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,2461153.7916,13.33,0.05,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 20260423.2916 13.33CV 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 23.2916 2461153.7916 13.41 11:00:48.30 +03:22:38.3
250.05462 54.46736 galactic Leo Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.189 Phthia 0 0 0 13.5 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:00:48.30 +03:22:38.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:00:48.30 +03:22:38.3: 15.99 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 23.2916* 11 00 48.30 +03 22 38.3 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7916,13.41,0.05,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 20260423.2916 13.41CV 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 23.2916 2461153.7916 13.62 10:59:37.70 +10:44:59.9
239.44311 59.02753 galactic Leo Second-epoch detections are separated by 0.6" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.140 Siwa -0 0 0 13.4 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 10:59:37.70 +10:44:59.9: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 10:59:37.70 +10:44:59.9: 15.91 +/- 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 23.2916* 10 59 37.70 +10 44 59.9 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7916,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2916 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.2916 2461153.7916 13.94 11:02:54.68 +09:00:38.8
243.06208 58.61599 galactic Leo Second-epoch detections are separated by 0.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.90 Antiope -1 1 2 14.1 0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:02:54.68 +09:00:38.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:02:54.68 +09:00:38.8: 15.94 +/- 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 23.2916* 11 02 54.68 +09 00 38.8 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7916,13.94,0.05,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 20260423.2916 13.94CV 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 23.2916 2461153.7916 14.53 11:24:01.02 +01:57:30.3
259.46804 57.25887 galactic Leo Second-epoch detections are separated by 0.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.327 Columbia 2 0 2 14.6 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:24:01.02 +01:57:30.3: 15.83 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:24:01.02 +01:57:30.3: 15.82 +/- 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 23.2916* 11 24 01.02 +01 57 30.3 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7916,14.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2916 14.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.2916 2461153.7916 14.58 11:03:33.63 +10:46:46.5
240.51785 59.82424 galactic Leo Second-epoch detections are separated by 1.2" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.534 Nassovia -0 0 1 14.5 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:03:33.63 +10:46:46.5: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:03:33.63 +10:46:46.5: 15.88 +/- 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 23.2916* 11 03 33.63 +10 46 46.5 14.6 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,2461153.7916,14.58,0.05,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 20260423.2916 14.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 23.2916 2461153.7916 14.67 11:26:51.28 +09:43:16.0
250.03058 63.52597 galactic Leo Second-epoch detections are separated by 1.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.627 Charis 0 1 1 14.8 0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits at 11:26:51.28 +09:43:16.0: 15.80 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits at 11:26:51.28 +09:43:16.0: 15.87 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 23.2916* 11 26 51.28 +09 43 16.0 14.7 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,2461153.7916,14.67,0.05,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 20260423.2916 14.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461153.79195209 23.04.2026 07:00:14.661 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 5642
Objects passed selection criteria: 5632
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: 5140
Average stars matched: 5001.25 (97.3006 %)
Memory usage VmPeak: 111436 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 Thu Apr 23 02:25:29 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: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
First image: 2461082.88537814 11.02.2026 09:14:46.671 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Last image: 2461153.79195209 23.04.2026 07:00:14.661 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 31209
Objects passed selection criteria: 31120
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: 29335.2
Average stars matched: 28272 (96.3755 %)
Memory usage VmPeak: 132464 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 Thu Apr 23 02:27:12 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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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: 2461153.79118733
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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
Saving wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
Saving wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits'
wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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: 11:08:11.175 +05:59:37.65 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-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Image size: 941.4'x626.8' 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: 11:08:34.427 +05:58:13.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:34.427 +05:58:13.54
Angular distance between the image centers 0.0991 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Image size: 941.4'x626.8' 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: 11:08:32.121 +05:58:42.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:32.121 +05:58:42.22
Angular distance between the image centers 0.0882 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 11:08:34.427 +05:58:13.54
Second-epoch second image center 11:08:32.121 +05:58:42.22
Angular distance between the image centers 0.01244 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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.QLT7xwygCx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.NlaKvPiFOe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits &> /tmp/tmp.7X4YaSPIgX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits &> /tmp/tmp.w9IL8DpEsH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat' -> 'wcsmag.cat'
Read 5629 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0658 to 175.0329 deg, Dec +0.7091 to +11.2821 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 159.0658 to 175.0329 deg, Dec 0.7091 to 11.2821 deg
Loaded 3938 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): 3214 out of 3354 total matches.
Matched with Tycho-2 3354 out of 5629 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.832371
a=0.000000 b=1.000000 c=22.832371
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5629 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0658 to 175.0329 deg, Dec +0.7091 to +11.2821 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 159.0658 to 175.0329 deg, Dec 0.7091 to 11.2821 deg
Loaded 3938 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): 3214 out of 3354 total matches.
Matched with Tycho-2 3354 out of 5629 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits (aperture=6.3)
Read 5671 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0797 to 175.0433 deg, Dec +0.7091 to +11.2820 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 159.0797 to 175.0433 deg, Dec 0.7091 to 11.2820 deg
Loaded 3931 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): 3189 out of 3352 total matches.
Matched with Tycho-2 3352 out of 5671 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.1 pix Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
2.1 pix fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
2.1 pix wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.1 pix wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Limiting magnitude estimates:
15.2 mag. Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.2 mag. Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.0 mag. fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
14.9 mag. fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.9 (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.QLT7xwygCx (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=5629
Got 5629 stars (including 5225 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 5629 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.NlaKvPiFOe (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=431, passed=5671
Got 5671 stars (including 5234 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 5671 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 5584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.7X4YaSPIgX (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=334, passed=4778
Got 4778 stars (including 4437 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat
util/solve_plate_with_UCAC5 got 4778 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 450 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 4706 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 450 to 510 (Dec 0.2 to 11.6)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 4706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 4706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.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.w9IL8DpEsH (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=324, passed=4609
Got 4609 stars (including 4280 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat
util/solve_plate_with_UCAC5 got 4609 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits'
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20437.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20431_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 20431_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20437_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 20437_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20459_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 20459_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:23:23.26 +06:07:13.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 9s
Prepared the HTML report for the field Leo-07-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 ####
11:02:00.05 +04:59:17.8
11:25:38.98 +06:01:43.2
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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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: 11:08:11.175 +05:59:37.65 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-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Image size: 941.4'x626.8' 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: 11:08:34.427 +05:58:13.54 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:34.427 +05:58:13.54
Angular distance between the image centers 0.0991 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Image size: 941.4'x626.8' 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: 11:08:32.121 +05:58:42.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:11.175 +05:59:37.65
Second-epoch image center 11:08:32.121 +05:58:42.22
Angular distance between the image centers 0.0882 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 11:08:34.427 +05:58:13.54
Second-epoch second image center 11:08:32.121 +05:58:42.22
Angular distance between the image centers 0.01244 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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits &> /tmp/tmp.gHFZIPLy8K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits &> /tmp/tmp.XMFgbg2ZUb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits &> /tmp/tmp.ifcqeER9nj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits &> /tmp/tmp.xG41JgLsqB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
Found non-empty wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits and wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
The reference image (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat) found
'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat' -> 'wcsmag.cat'
Read 31032 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0537 to 175.0351 deg, Dec +0.7036 to +11.2819 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 159.0537 to 175.0351 deg, Dec 0.7036 to 11.2819 deg
Loaded 3942 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): 3142 out of 3441 total matches.
Matched with Tycho-2 3441 out of 31032 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.714936
a=0.000000 b=1.000000 c=22.714936
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31032 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0537 to 175.0351 deg, Dec +0.7036 to +11.2819 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 159.0537 to 175.0351 deg, Dec 0.7036 to 11.2819 deg
Loaded 3942 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): 3142 out of 3441 total matches.
Matched with Tycho-2 3441 out of 31032 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits (aperture=5.0)
Read 31414 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.0562 to 175.0433 deg, Dec +0.7025 to +11.2818 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 159.0562 to 175.0433 deg, Dec 0.7025 to 11.2818 deg
Loaded 3941 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): 3120 out of 3437 total matches.
Matched with Tycho-2 3437 out of 31414 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.0 pix Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
2.0 pix fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
2.0 pix fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
2.0 pix wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
2.0 pix wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Limiting magnitude estimates:
15.3 mag. Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
15.3 mag. Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
15.2 mag. fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
15.1 mag. fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (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.gHFZIPLy8K (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1190, passed=31016
Got 31016 stars (including 29781 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat
util/solve_plate_with_UCAC5 got 31016 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 30732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-14-46_20.00sec_-14.90C_LIGHT_0423.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.XMFgbg2ZUb (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits' -> 'wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat corresponding to the image wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1251, passed=31400
Got 31400 stars (including 30103 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat
util/solve_plate_with_UCAC5 got 31400 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 31074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits -region wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-02-11_03-15-32_20.00sec_-15.00C_LIGHT_0424.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.ifcqeER9nj (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=916, passed=28120
Got 28120 stars (including 27158 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat
util/solve_plate_with_UCAC5 got 28120 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 27812 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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 27812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 27812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.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.xG41JgLsqB (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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=956, passed=27627
Got 27627 stars (including 26617 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat
util/solve_plate_with_UCAC5 got 27627 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 27206 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 450 to 510 (Dec 0.2 to 11.7)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 27207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 27207 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits -region wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/wcs_fd_Leo-07-Q1b1x1_2026-04-23_01-59-08_20.00sec_-4.90C_LIGHTs_0135.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.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_2026-04-23_CI_Leo-07-Q1b1x1_020108_TTUQ1b1x1_710832_Z18QOEXt/wcs_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136.fits
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53153.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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: 7s
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Considering the candidate 52324_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52324_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:13:28.64 +07:15:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52326_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52326_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:18:30.14 +10:50:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52461_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52461_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:02:00.04 +04:59:17.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52469_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52469_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:25:38.97 +06:01:43.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52559_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52559_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52571_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52571_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:40:59.64 +05:47:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52608_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52608_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52618_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52618_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:50:09.94 +08:50:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52624_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52624_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:42:39.14 +03:33:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52697_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52697_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:18:56.45 +10:11:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52704_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52704_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52711_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52711_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52744_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52744_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52748_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52748_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:06:16.30 +07:50:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52765_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52765_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:50:45.25 +06:57:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52771_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52771_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:04:58.18 +07:22:12.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52775_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52775_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:07:23.29 +06:22:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52809_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52809_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52821_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52821_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:10:21.03 +11:03:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52878_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52878_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:03:50.60 +05:56:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52906_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52906_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:48:17.11 +02:47:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52913_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 52913_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 52942_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52942_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:21:07.37 +07:22:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52997_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 52997_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:09:15.43 +04:41:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53102_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 53102_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 53127_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53127_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:47:58.38 +06:54:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53133_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 53133_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 53153_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
Preparing report for the candidate 53153_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
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Considering the candidate 53183_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53183_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:36:56.26 +07:20:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53201_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53201_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:08:35.14 +10:10:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.365 3867406638873432704 167.14614429010 +10.16725977221 15.5067 15.0204 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53212_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53212_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:05:29.63 +04:04:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.67, MAG_FAINT_SEARCH_LIMIT=15.65)GAIADR2_OUTPUT=# 1.244 3815010546123266688 166.37334357075 +04.08031286954 14.8849 14.2788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53214_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53214_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:54:50.75 +05:50:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 3.238 3864261344127626240 163.71232888368 +05.84042329364 14.6591 14.1111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53222_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53222_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:45:55.76 +03:40:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 0.831 3857537731740065280 161.48212351388 +03.68276371097 15.3261 14.9384 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53233_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53233_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:50:01.08 +06:32:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53279_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53279_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 10:39:42.05 +07:55:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53285_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53285_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
**** FOUND 11:09:14.62 +10:05:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.716 3867359566031865984 167.31093639300 +10.09663526938 14.8861 14.3599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53312_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136
The candidate 53312_fd_Leo-07-Q1b1x1_2026-04-23_02-00-14_20.00sec_-4.90C_LIGHTs_0136 did not pass the final checks
