This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf
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 06 18.1945 2461209.6945 12.49 11:23:51.32 +03:18:32.6
257.83314 58.29135 galactic Leo Second-epoch detections are separated by 0.4" and 8.3 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 12.9 0 -0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:23:51.32 +03:18:32.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:23:51.32 +03:18:32.6: 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 06 18.1945* 11 23 51.32 +03 18 32.6 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 12.49CV 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 06 18.1945 2461209.6945 13.21 11:02:34.13 +03:33:04.8
250.37770 54.90226 galactic Leo Second-epoch detections are separated by 2.1" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.35 Leukothea 0 -0 0 13.6 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:02:34.13 +03:33:04.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:02:34.13 +03:33:04.8: 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 06 18.1945* 11 02 34.13 +03 33 04.8 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,2461209.6945,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 13.21CV 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 06 18.1945 2461209.6945 13.56 11:16:43.47 +02:19:30.5
256.45847 56.39699 galactic Leo Second-epoch detections are separated by 1.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.270 Anahita 0 -0 0 13.8 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:16:43.47 +02:19:30.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:16:43.47 +02:19:30.5: 15.79 +/- 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 06 18.1945* 11 16 43.47 +02 19 30.5 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,2461209.6945,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.1945 2461209.6945 13.74 11:06:20.11 +03:51:39.1
251.16732 55.78378 galactic Leo Second-epoch detections are separated by 1.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.356 Liguria 1 1 1 14.0 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:06:20.11 +03:51:39.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:06:20.11 +03:51:39.1: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.1945* 11 06 20.11 +03 51 39.1 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 13.74CV 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 06 18.1945 2461209.6945 13.99 11:29:08.28 +02:30:58.4
260.74746 58.47738 galactic Leo Second-epoch detections are separated by 0.9" and 8.3 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 1 1 14.4 0 -0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:29:08.28 +02:30:58.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:29:08.28 +02:30:58.4: 15.71 +/- 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 06 18.1945* 11 29 08.28 +02 30 58.4 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.1945 2461209.6945 14.07 11:17:08.30 +08:02:11.5
249.08999 60.62705 galactic Leo Second-epoch detections are separated by 2.0" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.140 Siwa 0 0 1 14.1 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:17:08.30 +08:02:11.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:17:08.30 +08:02:11.5: 15.93 +/- 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 06 18.1945* 11 17 08.30 +08 02 11.5 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.1945 2461209.6945 14.05 11:00:44.77 +02:07:30.4
251.53611 53.56698 galactic Leo Second-epoch detections are separated by 1.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.336 Lacadiera 0 -0 0 14.5 0 -0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:00:44.77 +02:07:30.4: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:00:44.77 +02:07:30.4: 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 06 18.1945* 11 00 44.77 +02 07 30.4 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 14.05CV 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 06 18.1945 2461209.6945 14.27 11:13:25.59 +05:59:55.9
250.70520 58.54561 galactic Leo Second-epoch detections are separated by 0.4" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.136 Austria 0 -0 0 14.6 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:13:25.59 +05:59:55.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:13:25.59 +05:59:55.9: 15.96 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 18.1945* 11 13 25.59 +05 59 55.9 14.3 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 14.27CV 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 06 18.1945 2461209.6945 14.12 10:52:38.62 +04:12:36.2
246.64461 53.55928 galactic Leo Second-epoch detections are separated by 1.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.554 Peraga -1 0 1 14.4 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:52:38.62 +04:12:36.2: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:52:38.62 +04:12:36.2: 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 06 18.1945* 10 52 38.62 +04 12 36.2 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6945,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 18.1945 2461209.6945 14.41 11:15:22.24 +06:58:03.8
250.02514 59.57015 galactic Leo Second-epoch detections are separated by 0.7" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.90 Antiope 0 -0 0 14.7 -0 0
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:15:22.24 +06:58:03.8: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:15:22.24 +06:58:03.8: 15.95 +/- 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 06 18.1945* 11 15 22.24 +06 58 03.8 14.4 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,2461209.6945,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1945 14.41CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
First image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Last image: 2461209.69478464 18.06.2026 04:40:19.393 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.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.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4004
Objects passed selection criteria: 4003
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: 3754.25
Average stars matched: 3686 (98.1821 %)
Memory usage VmPeak: 110692 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 00:33:27 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: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
First image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Last image: 2461209.69478464 18.06.2026 04:40:19.393 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 34
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 21 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): 22265
Objects passed selection criteria: 22215
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: 21023.8
Average stars matched: 20322 (96.6621 %)
Memory usage VmPeak: 127816 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jun 16 15:05:04 CDT 2026
VaST build number 1.0rc89-100-g8a7e82c2
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jun 18 00:35:20 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.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: 2461209.69420953
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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits exists and is non-empty
Saving wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits to local_wcs_cache/
'wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits exists and is non-empty
Saving wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits to local_wcs_cache/
'wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits'
wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits exists and is non-empty
Saving wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (1st reference image)
verification OK: wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:41.744 +05:57:39.30 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:49.371 +06:02:00.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:41.744 +05:57:39.30
Second-epoch image center 11:08:49.371 +06:02:00.19
Angular distance between the image centers 0.0791 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:52.078 +06:01:32.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:41.744 +05:57:39.30
Second-epoch image center 11:08:52.078 +06:01:32.52
Angular distance between the image centers 0.0777 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 11:08:49.371 +06:02:00.19
Second-epoch second image center 11:08:52.078 +06:01:32.52
Angular distance between the image centers 0.01360 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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits &> /tmp/tmp.gs5ie44qvF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits &> /tmp/tmp.ZLkzxi0c6U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits &> /tmp/tmp.bppcjlqWRf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits &> /tmp/tmp.EqLUk9ZEYL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Found non-empty wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
The reference image (wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits) and catalog (wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat) found
'wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat' -> 'wcsmag.cat'
Read 5626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1365 to 175.0745 deg, Dec +0.5737 to +11.2590 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 159.1365 to 175.0745 deg, Dec 0.5737 to 11.2590 deg
Loaded 3954 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): 3201 out of 3312 total matches.
Matched with Tycho-2 3312 out of 5626 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.762800
a=0.000000 b=1.000000 c=22.762800
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.11
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.11
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1365 to 175.0745 deg, Dec +0.5737 to +11.2590 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 159.1365 to 175.0745 deg, Dec 0.5737 to 11.2590 deg
Loaded 3954 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): 3201 out of 3312 total matches.
Matched with Tycho-2 3312 out of 5626 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits:
Forced-photometry filter: calibrated wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -> calib.txt_param_ref_wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (aperture=6.5)
Read 5579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1771 to 175.0846 deg, Dec +0.7335 to +11.2823 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 159.1771 to 175.0846 deg, Dec 0.7335 to 11.2823 deg
Loaded 3902 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): 3209 out of 3301 total matches.
Matched with Tycho-2 3301 out of 5579 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits:
Forced-photometry filter: calibrated wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -> calib.txt_param_ref_wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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:
2.4 pix Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.3 pix Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
2.3 pix fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
2.3 pix fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
2.4 pix wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.3 pix wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Limiting magnitude estimates:
15.1 mag. Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
15.1 mag. Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
14.8 mag. fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
14.7 mag. fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
All-image limiting magnitude estimate: 14.7 (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.gs5ie44qvF (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=5626
Got 5626 stars (including 5255 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 5626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
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(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 452 to 508 (Dec 0.6 to 11.3)
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(), 5543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits N_match=943 sigma_overall_arcsec=0.504 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.520 sigma_q3_arcsec=0.509 sigma_q4_arcsec=0.476 n_q1=239 n_q2=269 n_q3=213 n_q4=222 worst_quadrant_to_overall_ratio=1.031
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -region wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ZLkzxi0c6U (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, passed=5576
Got 5576 stars (including 5240 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
util/solve_plate_with_UCAC5 got 5576 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5497 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
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(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits N_match=943 sigma_overall_arcsec=0.490 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.577 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.595 n_q1=234 n_q2=264 n_q3=219 n_q4=226 worst_quadrant_to_overall_ratio=1.214
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -region wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bppcjlqWRf (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=253, passed=4265
Got 4265 stars (including 4006 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 4265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4191 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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits N_match=947 sigma_overall_arcsec=0.428 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.525 sigma_q3_arcsec=0.396 sigma_q4_arcsec=0.489 n_q1=253 n_q2=256 n_q3=226 n_q4=212 worst_quadrant_to_overall_ratio=1.226
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits -region wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EqLUk9ZEYL (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=256, passed=4265
Got 4265 stars (including 4006 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 4265 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 4198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits N_match=947 sigma_overall_arcsec=0.420 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.505 sigma_q3_arcsec=0.387 sigma_q4_arcsec=0.436 n_q1=252 n_q2=254 n_q3=228 n_q4=213 worst_quadrant_to_overall_ratio=1.202
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits -region wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits sigma_overall=0.504 worst_q_ratio=1.031
ref2=Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits sigma_overall=0.490 worst_q_ratio=1.214
new1=fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits sigma_overall=0.428 worst_q_ratio=1.226
new2=fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits sigma_overall=0.420 worst_q_ratio=1.202
reference average sigma_overall=0.497 worst_q_ratio=1.1225
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503_astrometric_residuals.png (943 matched stars from wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148_astrometric_residuals.png (943 matched stars from wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070_astrometric_residuals.png (947 matched stars from wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071_astrometric_residuals.png (947 matched stars from wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits'
Preparing the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:33:01.12 +09:37:21.0: 11.05 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:07:35.62 +06:31:44.3: 12.08 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:10:25.13 +06:19:56.1: 12.18 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:10:25.13 +06:19:56.1: 12.15 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:33:01.12 +09:37:21.0: 11.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry reference-image weighted average: 11.12 +/- 0.00
Forced photometry filter REJECTED candidate at 11:10:25.13 +06:19:56.1: ref_mag=12.16 +/- 0.01 new_mean_mag=12.1326 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 11:33:01.12 +09:37:21.0: ref_mag=11.12 +/- 0.00 new_mean_mag=11.3532 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:07:35.62 +06:31:44.3: 12.06 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.07 +/- 0.01
Forced photometry filter REJECTED candidate at 11:07:35.62 +06:31:44.3: ref_mag=12.07 +/- 0.01 new_mean_mag=12.0305 delta=0.04 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20250_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 20250_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20262_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 20262_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20264_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 20264_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits exists and is non-empty
wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits exists and is non-empty
wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (1st reference image)
verification OK: wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Image size: 937.4'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:41.744 +05:57:39.30 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:49.371 +06:02:00.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:41.744 +05:57:39.30
Second-epoch image center 11:08:49.371 +06:02:00.19
Angular distance between the image centers 0.0791 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Image size: 937.6'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:52.078 +06:01:32.52 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:41.744 +05:57:39.30
Second-epoch image center 11:08:52.078 +06:01:32.52
Angular distance between the image centers 0.0777 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 11:08:49.371 +06:02:00.19
Second-epoch second image center 11:08:52.078 +06:01:32.52
Angular distance between the image centers 0.01360 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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits &> /tmp/tmp.oRt0usbyIw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits &> /tmp/tmp.I4gXgpWj2o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits &> /tmp/tmp.L2l39RpEHu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits &> /tmp/tmp.tLtG01BVn8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Found non-empty wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
The reference image (wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits) and catalog (wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat) found
'wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat' -> 'wcsmag.cat'
Read 29706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1354 to 175.0757 deg, Dec +0.5737 to +11.2606 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 159.1354 to 175.0757 deg, Dec 0.5737 to 11.2606 deg
Loaded 3956 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): 3140 out of 3393 total matches.
Matched with Tycho-2 3393 out of 29706 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.633700
a=0.000000 b=1.000000 c=22.633700
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1354 to 175.0757 deg, Dec +0.5737 to +11.2606 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 159.1354 to 175.0757 deg, Dec 0.5737 to 11.2606 deg
Loaded 3956 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): 3140 out of 3393 total matches.
Matched with Tycho-2 3393 out of 29706 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits:
Forced-photometry filter: calibrated wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -> calib.txt_param_ref_wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (aperture=5.0)
Read 29098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1771 to 175.0866 deg, Dec +0.7306 to +11.2850 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 159.1771 to 175.0866 deg, Dec 0.7306 to 11.2850 deg
Loaded 3903 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): 3156 out of 3385 total matches.
Matched with Tycho-2 3385 out of 29098 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits:
Forced-photometry filter: calibrated wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -> calib.txt_param_ref_wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.2 pix Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
2.2 pix fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
2.2 pix fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
2.2 pix wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.2 pix wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Limiting magnitude estimates:
15.3 mag. Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
15.3 mag. Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
14.9 mag. fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
14.8 mag. fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.3 (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.oRt0usbyIw (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.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-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1187, passed=29691
Got 29691 stars (including 28463 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 29691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 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(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 29432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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 452 to 508 (Dec 0.6 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(), 29432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 29432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits N_match=946 sigma_overall_arcsec=0.482 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.508 sigma_q3_arcsec=0.476 sigma_q4_arcsec=0.475 n_q1=228 n_q2=272 n_q3=220 n_q4=226 worst_quadrant_to_overall_ratio=1.053
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -region wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.I4gXgpWj2o (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.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-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Checking if the catalog wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS catalog name: wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1226, passed=29086
Got 29086 stars (including 27828 good ones) from the SExtractor catalog wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
util/solve_plate_with_UCAC5 got 29086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 28816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 28814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 28814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits N_match=949 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.560 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.569 n_q1=235 n_q2=261 n_q3=225 n_q4=228 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -region wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.L2l39RpEHu (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1010, passed=22211
Got 22211 stars (including 21169 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat
util/solve_plate_with_UCAC5 got 22211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21904 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 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(), 21902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits N_match=944 sigma_overall_arcsec=0.425 sigma_q1_arcsec=0.368 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.410 sigma_q4_arcsec=0.471 n_q1=261 n_q2=241 n_q3=238 n_q4=204 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits -region wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tLtG01BVn8 (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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Checking if the catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
WCS catalog name: wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=927, passed=21760
Got 21760 stars (including 20814 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat
util/solve_plate_with_UCAC5 got 21760 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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(), 21509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 21509 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits N_match=944 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.345 sigma_q2_arcsec=0.502 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.454 n_q1=261 n_q2=243 n_q3=234 n_q4=206 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits -region wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-39-29_20.00sec_4.90C_LIGHT_0070.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.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_2026-06-17_CI_Leo-07-Q2b1x1_234607_TTUQ2b1x1_4192715_pfRzKZBf/wcs_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071.fits
Preparing the HTML report for the field Leo-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:06:20.11 +03:51:39.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:23:51.32 +03:18:32.6: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:17:48.35 +03:51:37.3: 13.13 +/- 0.03 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:33:01.12 +09:37:20.8: 11.32 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:02:34.13 +03:33:04.8: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:16:43.47 +02:19:30.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:17:48.35 +03:51:37.3: 13.05 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
Forced photometry filter REJECTED candidate at 11:17:48.35 +03:51:37.3: ref_mag=13.08 +/- 0.02 new_mean_mag=13.1608 delta=-0.08 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:02:34.13 +03:33:04.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:29:08.28 +02:30:58.4: 15.74 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:06:20.11 +03:51:39.1: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:16:43.47 +02:19:30.5: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:33:01.12 +09:37:20.8: 11.38 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:23:51.32 +03:18:32.6: 15.82 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.35 +/- 0.00
Forced photometry filter REJECTED candidate at 11:33:01.12 +09:37:20.8: ref_mag=11.35 +/- 0.00 new_mean_mag=11.5132 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:17:08.30 +08:02:11.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:00:44.77 +02:07:30.4: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:13:25.59 +05:59:55.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:29:08.28 +02:30:58.4: 15.71 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:00:44.77 +02:07:30.4: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:17:08.30 +08:02:11.5: 15.93 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:13:25.59 +05:59:55.9: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:52:38.62 +04:12:36.2: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:26:24.21 +05:53:33.5: 15.07 +/- 0.19 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:52:38.62 +04:12:36.2: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:26:24.21 +05:53:33.5: 15.19 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.14
Forced photometry filter REJECTED candidate at 11:26:24.21 +05:53:33.5: ref_mag=15.13 +/- 0.14 new_mean_mag=14.5952 delta=0.53 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:15:22.24 +06:58:03.8: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:15:22.24 +06:58:03.8: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:35:46.56 +10:02:38.3: 15.06 +/- 0.22 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:24:07.74 +04:23:08.0: 14.73 +/- 0.13 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:35:46.56 +10:02:38.3: 14.93 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.14
Forced photometry filter REJECTED candidate at 11:35:46.56 +10:02:38.3: ref_mag=14.99 +/- 0.14 new_mean_mag=14.8526 delta=0.13 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:28:03.07 +02:14:03.0: 15.06 +/- 0.20 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:24:07.74 +04:23:08.0: 14.87 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.79 +/- 0.10
Forced photometry filter REJECTED candidate at 11:24:07.74 +04:23:08.0: ref_mag=14.79 +/- 0.10 new_mean_mag=14.5245 delta=0.26 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:28:03.07 +02:14:03.0: 15.03 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.14
Forced photometry filter REJECTED candidate at 11:28:03.07 +02:14:03.0: ref_mag=15.04 +/- 0.14 new_mean_mag=14.7940 delta=0.25 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:28:14.66 +04:36:39.0: 14.87 +/- 0.16 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:36:22.91 +07:19:32.1: 14.65 +/- 0.14 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:16:40.74 +04:42:40.1: 15.10 +/- 0.17 detection
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:28:14.66 +04:36:39.0: 14.92 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.90 +/- 0.11
Forced photometry filter REJECTED candidate at 11:28:14.66 +04:36:39.0: ref_mag=14.90 +/- 0.11 new_mean_mag=14.8400 delta=0.06 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:36:22.91 +07:19:32.1: 15.00 +/- 0.19 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.11
Forced photometry filter REJECTED candidate at 11:36:22.91 +07:19:32.1: ref_mag=14.77 +/- 0.11 new_mean_mag=14.6628 delta=0.11 (need > 0.90)
Forced photometry on wcs_Leo-07-Q2b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:16:40.74 +04:42:40.1: 15.01 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.12
Forced photometry filter REJECTED candidate at 11:16:40.74 +04:42:40.1: ref_mag=15.05 +/- 0.12 new_mean_mag=14.7625 delta=0.29 (need > 0.90)
Adding exclusion_list_local.txt__out32189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32276.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32337.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 8s
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Considering the candidate 32166_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32166_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32189_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32189_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32210_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32210_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32221_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32221_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32223_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32223_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
**** FOUND 11:21:16.93 +06:01:25.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 32237_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32237_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
**** FOUND 11:04:58.16 +07:22:12.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32239_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32239_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32255_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32255_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
**** FOUND 11:06:59.50 +01:56:44.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32258_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32258_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32265_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32265_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
**** FOUND 11:21:07.40 +07:22:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32273_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32273_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32276_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32276_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32285_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32285_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32295_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32295_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32302_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32302_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32324_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32324_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32337_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
Preparing report for the candidate 32337_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
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Considering the candidate 32364_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32364_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32371_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32371_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32373_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32373_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32397_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32397_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32402_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32402_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
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Considering the candidate 32408_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071
The candidate 32408_fd_Leo-07-Q2b1x1_2026-06-17_23-40-19_20.00sec_4.90C_LIGHT_0071 did not pass the final checks
