This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 28.4551 2461158.9551 12.15 16:18:21.67 -13:54:06.0
0.30109 25.18370 galactic Sco Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.346 Hermentaria 1 -0 1 11.9 -0 0
Forced photometry on wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits at 16:18:21.67 -13:54:06.0: 15.22 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits at 16:18:21.67 -13:54:06.0: 15.28 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461158.9551,12.15,0.05,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 20260428.4551 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4551 2461158.9551 11.46 15:47:24.05 -20:56:13.1
349.02346 25.79074 galactic Sco Second-epoch detections are separated by 0.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.70 Panopaea -0 -2 2 11.4 -0 -0
Forced photometry on wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits at 15:47:24.05 -20:56:13.1: 15.16 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits at 15:47:24.05 -20:56:13.1: 15.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461158.9551,11.46,0.05,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 20260428.4551 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.4551 2461158.9551 13.48 16:10:23.66 -13:54:11.8
358.91808 26.66386 galactic Sco Second-epoch detections are separated by 1.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.563 Suleika 1 0 1 13.5 -0 0
Forced photometry on wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits at 16:10:23.66 -13:54:11.8: 15.30 +/- 99.00 upperlimit
Forced photometry on wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits at 16:10:23.66 -13:54:11.8: 15.33 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461158.9551,13.48,0.05,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 20260428.4551 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
GR Lib,2461158.9551,9.83,0.05,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
GR Lib 20260428.4551 9.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ASAS J154445-1805.1,2461158.9551,11.87,0.05,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
ASAS J154445-1805.1 20260428.4551 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
NSVS J1603395-163025,2461158.9551,12.10,0.05,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
NSVS J1603395-163025 20260428.4551 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J154425-1709.5,2461158.9551,11.37,0.05,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
ASAS J154425-1709.5 20260428.4551 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
RR Lib,2461158.9551,11.33,0.05,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
RR Lib 20260428.4551 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Sco,2461158.9551,12.61,0.05,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
X Sco 20260428.4551 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ASAS J154124-2047.1,2461158.9551,10.88,0.05,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
ASAS J154124-2047.1 20260428.4551 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461126.93607301 27.03.2026 10:27:46.708 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
First image: 2461126.93607301 27.03.2026 10:27:46.708 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Last image: 2461158.95540961 28.04.2026 10:55:37.390 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 6 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): 6694
Objects passed selection criteria: 6676
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 4977.25
Average stars matched: 4624.5 (92.9128 %)
Memory usage VmPeak: 112136 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 28 06:49:37 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: 2461126.93607301 27.03.2026 10:27:46.708 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
First image: 2461126.93607301 27.03.2026 10:27:46.708 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Last image: 2461158.95540961 28.04.2026 10:55:37.390 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 seconds
Number of parallel threads: 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): 42850
Objects passed selection criteria: 42771
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 33173
Average stars matched: 29702 (89.5367 %)
Memory usage VmPeak: 141224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 28 06:51:37 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/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
SExtractor catalog cache: saved Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.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/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.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: 2461158.95483538
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_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits'
wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits'
wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits exists and is non-empty
Saving wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits to local_wcs_cache/
'wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits' -> 'local_wcs_cache/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits'
wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits exists and is non-empty
Saving wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits to local_wcs_cache/
'wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits' -> 'local_wcs_cache/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits (1st reference image)
verification OK: wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:00:00.942 -18:02:14.37 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_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits (1st new image)
verification OK: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Image size: 937.4'x624.4' 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: 15:59:58.903 -17:58:56.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:00:00.942 -18:02:14.37
Second-epoch image center 15:59:58.903 -17:58:56.78
Angular distance between the image centers 0.0555 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits (2nd new image)
verification OK: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Image size: 937.4'x624.4' 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: 15:59:58.591 -17:59:41.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:00:00.942 -18:02:14.37
Second-epoch image center 15:59:58.591 -17:59:41.33
Angular distance between the image centers 0.0435 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 15:59:58.903 -17:58:56.78
Second-epoch second image center 15:59:58.591 -17:59:41.33
Angular distance between the image centers 0.01244 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits &> /tmp/tmp.SmODsxBZIm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits &> /tmp/tmp.QfQfYl6ukg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits &> /tmp/tmp.k8HvbCuPHX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits &> /tmp/tmp.SGgjoYymX3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.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_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits and wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits and wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
Found non-empty wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits and wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
The reference image (wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits) and catalog (wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat) found
'wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Read 7268 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.5135 to 248.3948 deg, Dec -23.3115 to -12.6532 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 231.5135 to 248.3948 deg, Dec -23.3115 to -12.6532 deg
Loaded 5928 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): 4664 out of 4758 total matches.
Matched with Tycho-2 4758 out of 7268 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.590408
a=0.000000 b=1.000000 c=22.590408
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.53
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7268 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.5135 to 248.3948 deg, Dec -23.3115 to -12.6532 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 231.5135 to 248.3948 deg, Dec -23.3115 to -12.6532 deg
Loaded 5928 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): 4664 out of 4758 total matches.
Matched with Tycho-2 4758 out of 7268 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits -> calib.txt_param_ref_wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits (aperture=7.0)
Read 7283 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.4628 to 248.3946 deg, Dec -23.3115 to -12.6534 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 231.4628 to 248.3946 deg, Dec -23.3115 to -12.6534 deg
Loaded 5947 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): 4651 out of 4748 total matches.
Matched with Tycho-2 4748 out of 7283 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits -> calib.txt_param_ref_wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits (aperture=6.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.8 pix Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
2.6 pix Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
2.9 pix fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
2.8 pix fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
2.8 pix wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
2.6 pix wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Limiting magnitude estimates:
14.5 mag. Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
14.6 mag. Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
14.1 mag. fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
14.2 mag. fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.SmODsxBZIm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits' -> 'wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Checking if the catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
WCS catalog name: wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=312, passed=7268
Got 7268 stars (including 6952 good ones) from the SExtractor catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 7268 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits -region wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QfQfYl6ukg (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits' -> 'wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Checking if the catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
WCS catalog name: wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=342, passed=7283
Got 7283 stars (including 6934 good ones) from the SExtractor catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 7283 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7141 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 333 to 388 (Dec -23.3 to -12.7)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7140 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 7140 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits -region wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.k8HvbCuPHX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Checking if the catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
WCS catalog name: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=374, passed=4672
Got 4672 stars (including 4290 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat
util/solve_plate_with_UCAC5 got 4672 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 4506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 4508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 4504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits -region wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SGgjoYymX3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Checking if the catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
WCS catalog name: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=400, passed=4677
Got 4677 stars (including 4272 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 4677 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 4487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 4485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 4479 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 961 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits -region wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits'
Saving fully-calibrated image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits'
Preparing the HTML report for the field Lib-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21004.dat to exclusion_list_gaiadr2.txt
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 20303_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 20303_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:06:04.88 -17:46:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20436_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 20436_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:42:03.39 -21:10:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21004_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 21004_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:56:23.72 -18:18:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 0.510 6248320694264829440 239.09877246623 -18.30421281757 8.9288 7.5432 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05377_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 05377_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:14:46.97 -15:39:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20072_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 20072_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:02:05.82 -18:18:08.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lib-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
SExtractor catalog cache: saved Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.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_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits exists and is non-empty
wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits exists and is non-empty
wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits (1st reference image)
verification OK: wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Image size: 937.5'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 16:00:00.942 -18:02:14.37 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_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits (1st new image)
verification OK: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Image size: 937.4'x624.4' 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: 15:59:58.903 -17:58:56.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:00:00.942 -18:02:14.37
Second-epoch image center 15:59:58.903 -17:58:56.78
Angular distance between the image centers 0.0555 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits (2nd new image)
verification OK: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Image size: 937.4'x624.4' 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: 15:59:58.591 -17:59:41.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:00:00.942 -18:02:14.37
Second-epoch image center 15:59:58.591 -17:59:41.33
Angular distance between the image centers 0.0435 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 15:59:58.903 -17:58:56.78
Second-epoch second image center 15:59:58.591 -17:59:41.33
Angular distance between the image centers 0.01244 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits &> /tmp/tmp.bTModjx30K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits &> /tmp/tmp.LOVWBJj9UM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits &> /tmp/tmp.0MPwPeNiXH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits &> /tmp/tmp.LqAKyE2Ih2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.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_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits and wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits and wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
Found non-empty wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits and wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
The reference image (wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits) and catalog (wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat) found
'wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat' -> 'wcsmag.cat'
Read 45889 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.4646 to 248.4060 deg, Dec -23.3114 to -12.6097 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 231.4646 to 248.4060 deg, Dec -23.3114 to -12.6097 deg
Loaded 5971 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): 4816 out of 5211 total matches.
Matched with Tycho-2 5211 out of 45889 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.420596
a=0.000000 b=1.000000 c=22.420596
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.65
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 45889 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.4646 to 248.4060 deg, Dec -23.3114 to -12.6097 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 231.4646 to 248.4060 deg, Dec -23.3114 to -12.6097 deg
Loaded 5971 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): 4816 out of 5211 total matches.
Matched with Tycho-2 5211 out of 45889 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits -> calib.txt_param_ref_wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits (aperture=5.5)
Read 49079 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 231.4619 to 248.4047 deg, Dec -23.3127 to -12.6335 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 231.4619 to 248.4047 deg, Dec -23.3127 to -12.6335 deg
Loaded 5963 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): 4787 out of 5214 total matches.
Matched with Tycho-2 5214 out of 49079 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits -> calib.txt_param_ref_wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 35 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.8 pix Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
2.5 pix Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
2.8 pix fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
2.5 pix fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
2.8 pix wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
2.5 pix wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Limiting magnitude estimates:
14.7 mag. Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
14.7 mag. Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
14.2 mag. fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
14.3 mag. fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.bTModjx30K (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits' -> 'wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
Checking if the catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits
WCS catalog name: wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2373, passed=45884
Got 45884 stars (including 43453 good ones) from the SExtractor catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 45884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 45105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 45105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 45105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits -region wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-27-46_20.00sec_-14.90C_LIGHT_0482.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LOVWBJj9UM (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits' -> 'wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
Checking if the catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat corresponding to the image wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits
WCS catalog name: wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2436, passed=49071
Got 49071 stars (including 46573 good ones) from the SExtractor catalog wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 49071 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 48333 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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 48332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 48332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits -region wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-04-Q2b1x1_2026-03-27_05-28-29_20.00sec_-14.90C_LIGHT_0483.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0MPwPeNiXH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Checking if the catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
WCS catalog name: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2232, passed=29879
Got 29879 stars (including 27621 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat
util/solve_plate_with_UCAC5 got 29879 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 28757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 28757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 28712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 965 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits -region wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LqAKyE2Ih2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
WCS-calibrated image found: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Checking if the catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat corresponding to the image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
WCS catalog name: wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2452, passed=31633
Got 31633 stars (including 29146 good ones) from the SExtractor catalog wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 31633 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 30429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 30432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 30405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 966 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits -region wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-54-47_20.00sec_-4.90C_LIGHT_0320.fits
Saving fully-calibrated image wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-28_CI_Lib-04-Q2b1x1_060457_TTUQ2b1x1_310620_BWhVm3OI/wcs_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321.fits
Preparing the HTML report for the field Lib-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out14969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out59735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61493.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59703.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55053_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 55053_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:18:00.48 -18:21:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.099 6246255261670484736 244.50194300292 -18.35552498068 13.7767 12.9654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55059_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 55059_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:42:44.84 -13:47:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55064_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 55064_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:57:16.43 -18:32:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56176_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 56176_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56309_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 56309_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58488_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 58488_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:13:28.91 -21:11:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59703_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 59703_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 59735_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 59735_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:14:12.53 -19:20:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.301 6245608881973822464 243.55255289721 -19.34977252648 12.6779 11.4511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 60145_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 60145_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:07:22.11 -14:44:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60782_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 60782_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:11:21.64 -13:55:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.687 4329597518527310976 242.83997492381 -13.93051393833 14.5328 13.9565 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61493_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61493_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:10:44.75 -16:36:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.332 6249709549246536064 242.68740911505 -16.60103210622 12.4381 10.6642 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61535_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61535_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:16:12.43 -17:05:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61539_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61539_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:45:35.39 -20:49:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.696 6241656073250043008 236.39707289901 -20.82960106588 12.7976 11.3980 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61583_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61583_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:18:27.97 -17:17:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 0.143 6246477740976019456 244.61651630178 -17.28891302366 13.9982 13.4300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61618_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61618_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:14:59.80 -17:14:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 2.813 6249471951656992640 243.74989456616 -17.23855109159 14.2067 13.4559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61736_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61736_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:11:50.21 -15:00:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.128 4329182830844881664 242.95949023169 -15.00590047487 14.8098 14.2580 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61896_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 61896_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:13:10.58 -15:32:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62056_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 62056_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:18:34.06 -19:21:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.542 6245931352415999616 244.64197686838 -19.36430598291 13.7579 12.8030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62069_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 62069_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:00:10.25 -15:27:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.030 6262512709320915712 240.04277598333 -15.45236037576 13.8634 13.1006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62295_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 62295_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:48:16.55 -20:46:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.794 6241624286193856768 237.06822120063 -20.77755148655 12.6141 11.2733 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62455_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 62455_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:53:29.72 -18:11:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.251 6248521660074709376 238.37380602210 -18.19985180420 12.6071 11.2042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62490_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 62490_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:57:07.33 -15:27:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.989 6262687325510450048 239.28081753250 -15.46268018837 13.8932 13.1405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 14969_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 14969_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:41:42.64 -19:45:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 5.420 6253973554121015680 235.42622421698 -19.75362333177 11.6352 10.0453 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 41098_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 41098_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 32164_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 32164_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:43:24.57 -16:42:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21543_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 21543_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:02:05.82 -18:18:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44074_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 44074_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 15:51:39.47 -16:05:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22530_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 22530_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 45380_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 45380_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 27070_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 27070_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 21522_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 21522_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 07693_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
Preparing report for the candidate 07693_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
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Considering the candidate 06309_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 06309_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
**** FOUND 16:06:00.62 -21:43:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08684_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321
The candidate 08684_fd_Lib-04-Q2b1x1_2026-04-28_05-55-37_20.00sec_-4.90C_LIGHT_0321 did not pass the final checks
