This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.7861-16.4605,2461136.6330,11.50,0.05,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
ATO J089.7861-16.4605 20260406.1330 11.50CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2964116227017695872,2461136.6330,10.64,0.05,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
Gaia DR3 2964116227017695872 20260406.1330 10.64CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J055742-1916.3,2461136.6330,10.67,0.05,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 J055742-1916.3 20260406.1330 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AV Lep,2461136.6330,8.84,0.05,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
AV Lep 20260406.1330 8.84CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OZ CMa,2461136.6330,10.91,0.05,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
OZ CMa 20260406.1330 10.91CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6330,13.14,0.05,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
target 20260406.1330 13.14CV 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 06.1330 2461136.6330 11.85 05:47:24.72 -22:04:06.3
226.67449 -23.50007 galactic Lep Second-epoch detections are separated by 8.8" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2964115814696389248 | 05:47:25.31 -22:04:06.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2964115814696389248,2461136.6330,11.85,0.05,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
Large-amplitude variable Gaia DR2 2964115814696389248 20260406.1330 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2965944543053828992,2461136.6330,11.83,0.05,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
Gaia DR3 2965944543053828992 20260406.1330 11.83CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2994993434100167808,2461136.6330,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2994993434100167808 20260406.1330 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.0774-21.8300,2461136.6330,10.15,0.05,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
ATO J087.0774-21.8300 20260406.1330 10.15CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J055005.74-163223.8,2461136.6330,12.70,0.05,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
ASASSN-V J055005.74-163223.8 20260406.1330 12.70CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061808-1447.3,2461136.6330,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061808-1447.3 20260406.1330 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0610527-145942,2461136.6330,12.89,0.05,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 J0610527-145942 20260406.1330 12.89CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062052.13-164541.5,2461136.6330,13.35,0.05,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
ASASSN-V J062052.13-164541.5 20260406.1330 13.35CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J061528-1650.0,2461136.6330,9.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J061528-1650.0 20260406.1330 9.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J060210-1645.5,2461136.6330,11.39,0.05,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 J060210-1645.5 20260406.1330 11.39CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J055341-2013.9,2461136.6330,11.04,0.05,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 J055341-2013.9 20260406.1330 11.04CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0638114-141440,2461136.6330,12.72,0.05,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 J0638114-141440 20260406.1330 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J060151-2127.7,2461136.6330,10.34,0.05,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 J060151-2127.7 20260406.1330 10.34CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060721.13-151819.5,2461136.6330,13.16,0.05,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
ASASSN-V J060721.13-151819.5 20260406.1330 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.70844672 18.01.2026 04:59:59.797 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
First image: 2461058.70844672 18.01.2026 04:59:59.797 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Last image: 2461136.63329389 06.04.2026 03:11:46.592 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.95
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: 8 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): 15083
Objects passed selection criteria: 15031
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 12315.5
Average stars matched: 11299.5 (91.7502 %)
Memory usage VmPeak: 118500 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 22:14:07 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.70844672 18.01.2026 04:59:59.797 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
First image: 2461058.70844672 18.01.2026 04:59:59.797 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Last image: 2461136.63329389 06.04.2026 03:11:46.592 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 164
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 74 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): 99428
Objects passed selection criteria: 99171
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 77679
Average stars matched: 71469.2 (92.0059 %)
Memory usage VmPeak: 1945060 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 22:17:41 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/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
SExtractor catalog cache: saved CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat to cache
SExtractor catalog cache: saved CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.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/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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: 2461136.63272786
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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits exists and is non-empty
Saving wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits to local_wcs_cache/
'wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits' -> 'local_wcs_cache/wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits'
wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits exists and is non-empty
Saving wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits to local_wcs_cache/
'wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits'
wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits'
wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits exists and is non-empty
Saving wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits to local_wcs_cache/
'wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:20.181 -17:59:57.36
Second-epoch image center 06:13:20.011 -18:00:09.98
Angular distance between the image centers 0.0036 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:20.181 -17:59:57.36
Second-epoch image center 06:13:19.309 -17:59:43.15
Angular distance between the image centers 0.0052 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 06:13:20.011 -18:00:09.98
Second-epoch second image center 06:13:19.309 -17:59:43.15
Angular distance between the image centers 0.00796 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/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits &> /tmp/tmp.TCQQSvWhr7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits &> /tmp/tmp.56TSdVNWuW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits &> /tmp/tmp.Bsq8ruHxm0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits &> /tmp/tmp.tPm5zBZzGM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Calibrating the magnitude scale
Found non-empty wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits and wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits and wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
Found non-empty wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits and wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
The reference image (wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits) and catalog (wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat) found
'wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat' -> 'wcsmag.cat'
Read 16108 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.8225 to 101.8126 deg, Dec -23.2835 to -12.5977 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 84.8225 to 101.8126 deg, Dec -23.2835 to -12.5977 deg
Loaded 14935 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): 10846 out of 11501 total matches.
Matched with Tycho-2 11501 out of 16108 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.826981
a=0.000000 b=1.000000 c=22.826981
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
2.1 pix CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
3.2 pix fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
3.2 pix fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Limiting magnitude estimates:
14.9 mag. CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
14.9 mag. CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
14.3 mag. fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
14.3 mag. fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (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.TCQQSvWhr7 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits' -> 'wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WCS-calibrated image found: wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Checking if the catalog wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WCS catalog name: wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1454, passed=16108
Got 16108 stars (including 14633 good ones) from the SExtractor catalog wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 16108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (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...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (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
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits -region wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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.56TSdVNWuW (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits' -> 'wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WCS-calibrated image found: wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
Checking if the catalog wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WCS catalog name: wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1470, passed=16027
Got 16027 stars (including 14537 good ones) from the SExtractor catalog wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 16027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (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...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15695 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (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
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 15694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits -region wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.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.Bsq8ruHxm0 (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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
Checking if the catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
WCS catalog name: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1231, passed=12927
Got 12927 stars (including 11689 good ones) from the SExtractor catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 12927 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits -region wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.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.tPm5zBZzGM (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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Checking if the catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
WCS catalog name: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1250, passed=12867
Got 12867 stars (including 11608 good ones) from the SExtractor catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 12867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 12420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 12416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 12416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits -region wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits'
Saving fully-calibrated image wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits'
Saving fully-calibrated image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits'
Preparing the HTML report for the field CMa-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20769.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 4s
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Considering the candidate 20764_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 20764_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 20765_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 20765_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:25.90 -22:10:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)GAIADR2_OUTPUT=# 1.225 2917576098837086848 087.35825283285 -22.18016841990 10.5200 10.0358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20766_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 20766_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:18.32 -20:45:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 0.547 2965949250337954560 087.07636954209 -20.75423138674 10.3454 9.9056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20769_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 20769_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 20774_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 20774_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:18.85 -21:49:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 2.055 2965626784195838976 087.07798578860 -21.81735490682 9.3787 9.0297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21826_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 21826_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:19:38.91 -17:00:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22030_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 22030_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:34:26.77 -13:41:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22628_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 22628_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:13:40.01 -15:28:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.242 2992908107220542720 093.41675248495 -15.46903678663 11.3346 10.5934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22783_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 22783_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:02:09.91 -16:45:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 1.609 2991357933263295488 090.54083816708 -16.75894939646 10.6200 9.2695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23055_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 23055_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:30:54.72 -19:52:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.755 2939872511019376256 097.72801901398 -19.87365341942 11.6730 11.0071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23134_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 23134_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:30:59.87 -22:06:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.934 2937084527489208192 097.74932201012 -22.11024543717 11.8155 11.1651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23204_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 23204_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:30:59.76 -19:28:34.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)
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Considering the candidate 06185_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 06185_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 03312_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 03312_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 11310_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 11310_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 04841_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 04841_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:59:18.37 -20:13:25.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 26s
Prepared the HTML report for the field CMa-01-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 ####
06:01:51.02 -21:06:14.5
05:57:42.39 -19:16:19.0
06:29:57.94 -15:48:07.2
05:59:08.47 -16:27:52.6
05:48:03.54 -22:10:36.8
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/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
SExtractor catalog cache: saved CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat to cache
SExtractor catalog cache: saved CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Creating symlink local_wcs_cache/wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
Creating symlink local_wcs_cache/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits exists and is non-empty
wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits exists and is non-empty
wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits exists and is non-empty
wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:13:20.181 -17:59:57.36
Second-epoch image center 06:13:20.011 -18:00:09.98
Angular distance between the image centers 0.0036 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:13:20.181 -17:59:57.36
Second-epoch image center 06:13:19.309 -17:59:43.15
Angular distance between the image centers 0.0052 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 06:13:20.011 -18:00:09.98
Second-epoch second image center 06:13:19.309 -17:59:43.15
Angular distance between the image centers 0.00796 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/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits &> /tmp/tmp.aiy5VPS4VM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits &> /tmp/tmp.GrSHtbMA5V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits &> /tmp/tmp.18R7w3JTEf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits &> /tmp/tmp.7PJNOWkNdc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Calibrating the magnitude scale
Found non-empty wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits and wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits and wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
Found non-empty wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits and wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
The reference image (wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits) and catalog (wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat) found
'wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat' -> 'wcsmag.cat'
Read 110580 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 84.7847 to 101.8279 deg, Dec -23.2926 to -12.5861 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 84.7847 to 101.8279 deg, Dec -23.2926 to -12.5861 deg
Loaded 14996 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): 10576 out of 12761 total matches.
Matched with Tycho-2 12761 out of 110580 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.672477
a=0.000000 b=1.000000 c=22.672477
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 91 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
2.0 pix CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
3.1 pix fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
3.1 pix fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Limiting magnitude estimates:
15.0 mag. CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
15.0 mag. CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
14.3 mag. fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
14.3 mag. fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.8 (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.aiy5VPS4VM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits' -> 'wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WCS-calibrated image found: wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Checking if the catalog wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
WCS catalog name: wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=9180, passed=110560
Got 110560 stars (including 101197 good ones) from the SExtractor catalog wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 110560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 108988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 108990 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 108989 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits -region wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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.GrSHtbMA5V (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits' -> 'wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WCS-calibrated image found: wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
Checking if the catalog wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat corresponding to the image wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
WCS catalog name: wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=9420, passed=112088
Got 112088 stars (including 102477 good ones) from the SExtractor catalog wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 112088 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 111218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 111220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 111220 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits -region wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.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.18R7w3JTEf (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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
Checking if the catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
WCS catalog name: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=7729, passed=67052
Got 67052 stars (including 59251 good ones) from the SExtractor catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 67052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 64893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 64893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 64893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits -region wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.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.7PJNOWkNdc (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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Checking if the catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
WCS catalog name: wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=7855, passed=67536
Got 67536 stars (including 59628 good ones) from the SExtractor catalog wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 67536 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 65421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 65420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 65420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits -region wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_CMa-01-Q2b1x1_2026-01-17_22-59-59_20.00sec_-15.00C_LIGHT_0186.fits
Saving fully-calibrated image wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_CMa-01-Q2b1x1_2026-01-17_23-01-02_20.00sec_-14.90C_LIGHT_0187.fits
Saving fully-calibrated image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-10-57_20.00sec_-5.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.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_2026-04-05_CI_CMa-01-Q2b1x1_221226_TTUQ2b1x1_427_7hXFq0qC/wcs_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062.fits
Preparing the HTML report for the field CMa-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out121787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out128998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out139841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out143634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out128984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99144.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
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: 10s
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Considering the candidate 128947_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128947_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:35:55.29 -18:14:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.440 2940509609289448064 098.98079599932 -18.23417093996 14.2489 13.6190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128953_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128953_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:34:50.74 -14:54:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 0.551 2950347798816630784 098.71127843475 -14.90663004076 14.1596 13.6252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128958_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128958_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:08:00.08 -21:21:21.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 128964_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128964_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:51.43 -16:19:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 0.846 2994950411409967360 087.46419673883 -16.32252220910 12.6049 12.0051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128980_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128980_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:05:29.50 -22:01:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.374 2916972123357211776 091.37149426788 -22.02221663285 13.1235 12.5265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128983_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128983_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:26:11.05 -14:04:11.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 128984_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 128984_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 128992_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128992_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:45.24 -19:44:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.733 2966161146843728256 087.43860405749 -19.73930455900 12.3613 11.8915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128994_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128994_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:21.03 -20:16:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.938 2966074629022670464 087.08665858701 -20.26933214417 12.3965 11.9581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128998_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 128998_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:51.68 -19:49:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.459 2966156611358315904 087.21574274606 -19.81754304428 12.2604 11.7801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129000_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129000_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:56.79 -22:15:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.824 2917560018479522432 087.48715369926 -22.25356327366 12.1260 11.7013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129001_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129001_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:32.29 -16:45:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.467 2994901453080810112 087.13548651754 -16.75205183328 12.3557 11.9399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129004_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129004_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:51:40.91 -21:48:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.749 2917600902267868416 087.92044805357 -21.80145792389 12.1558 11.6278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129009_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129009_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:00.57 -22:14:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.428 2916071520252513664 087.00299900290 -22.23776497943 11.9868 11.4766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129010_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129010_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:06.80 -20:50:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.837 2965946261040732928 087.02954647411 -20.84316770170 11.9572 11.5704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129012_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129012_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:50:15.14 -21:55:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.035 2917585822642955776 087.56296812754 -21.93168368588 11.9320 11.4956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129014_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129014_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:50:17.02 -21:32:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.678 2965659151069556224 087.57064952436 -21.54197782356 11.9701 11.6728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129018_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129018_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:50:38.16 -22:01:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.285 2917572559783949184 087.65945373011 -22.03266355895 12.0537 11.6256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129022_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129022_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:51:51.58 -22:15:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.805 2917515316460091520 087.96479823061 -22.25482246277 12.0439 11.6001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129023_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129023_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:29:45.72 -18:25:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129025_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129025_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:40.70 -20:57:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.759 2965754224465017472 087.17066228132 -20.95625354499 11.9927 11.5961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129034_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129034_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:24:49.08 -14:58:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129042_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129042_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:07.83 -22:07:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.569 2964116467532381696 087.03292156094 -22.13347717948 11.5957 11.1638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129048_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129048_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:48.53 -20:00:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 2.967 2966149803831995648 087.20303359080 -20.00880706780 11.9841 11.2806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129053_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129053_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:35:50.08 -17:47:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129054_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129054_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:14.70 -17:23:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 4.260 2967843360977115136 087.06247626908 -17.38828642749 11.7493 11.2686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129056_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129056_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:51:07.08 -22:10:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 4.052 2917520259961930496 087.77848292720 -22.18050526631 11.5878 11.1537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129060_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129060_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:04.50 -21:54:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 4.306 2964124576433848704 087.02003766981 -21.91466268468 11.5622 11.2356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129061_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129061_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:00.25 -21:38:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 4.446 2965645024916192128 087.00236925179 -21.63781387816 11.5287 11.0801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129063_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 129063_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 129064_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129064_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:08.76 -21:53:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.389 2965622764102767360 087.28662594152 -21.89568782499 11.5016 11.1211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129076_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 129076_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 129077_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129077_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:38:05.03 -19:46:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129080_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129080_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:50:15.44 -22:02:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 4.968 2917573075180044672 087.56328782489 -22.04081583513 11.0339 10.6676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129081_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129081_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:50:20.93 -21:48:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 3.154 2917592076115310592 087.58633779904 -21.80575441150 11.2838 10.8947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129083_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129083_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:47:55.00 -17:28:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 2.526 2967819171720879616 086.97845597171 -17.47112435397 11.1064 10.7103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129084_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129084_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:48:22.60 -21:29:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 2.293 2965653275554036480 087.09416477892 -21.48333524619 11.1784 10.7512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129088_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129088_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:07.19 -16:35:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 3.166 2994909012223224960 087.27904245211 -16.59180343674 11.2142 10.7999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129090_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129090_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 129091_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129091_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 129095_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129095_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:50:22.85 -21:46:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 5.700 2917592488432161920 087.59407315101 -21.77048682967 10.6810 10.3120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129096_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129096_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:47:40.32 -21:52:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 2.953 2964136533622814976 086.91712813601 -21.87405154527 10.4268 9.9728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129100_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129100_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:49:26.06 -22:10:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.97, MAG_FAINT_SEARCH_LIMIT=11.95)GAIADR2_OUTPUT=# 1.121 2917576098837086848 087.35825283285 -22.18016841990 10.5200 10.0358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129101_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 129101_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 129104_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 129104_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 129108_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 129108_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 131057_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 131057_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:17:52.88 -16:48:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134456_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 134456_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:33:23.08 -15:33:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135897_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 135897_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:15:01.40 -20:17:13.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 137200_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 137200_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:27:01.59 -14:41:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137715_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 137715_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:23:43.95 -19:48:04.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 137778_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 137778_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:31:09.70 -16:37:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138731_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 138731_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:03:57.85 -13:55:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138757_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 138757_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:14:36.45 -22:14:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139053_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 139053_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:16:01.02 -17:01:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139201_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 139201_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:27:25.24 -15:19:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 5.431 2951009498658145792 096.85672741481 -15.31684375310 13.6512 12.9202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 139528_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 139528_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:31:36.50 -15:38:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139841_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 139841_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:22:16.60 -13:57:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.575 2999431509710285696 095.56900308640 -13.96387963745 13.9820 13.4332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140311_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 140311_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:28:26.65 -20:05:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.895 2939783106982334464 097.11157657945 -20.09971279638 13.4262 12.5638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140684_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 140684_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:37:51.83 -17:38:09.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 141011_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 141011_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:31:52.24 -19:05:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.077 2939986928947752448 097.96770840276 -19.09393552615 14.0861 13.3246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141537_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 141537_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:37:20.08 -19:21:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.914 2939504346425604224 099.33390966384 -19.35771498060 14.2760 13.8261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141809_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 141809_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:23:31.25 -21:14:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141890_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 141890_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:36:11.46 -19:38:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.930 2939474487813210240 099.04784888055 -19.64009250745 14.2815 13.6412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143083_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143083_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:37:12.29 -19:46:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 143359_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143359_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:32:14.01 -17:13:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 2.124 2943841610559768192 098.05828503089 -17.21825049670 14.4679 13.6709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143469_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143469_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:32:01.13 -14:42:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.256 2951163980042031616 098.00495972143 -14.70166700170 14.1729 13.4242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143472_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143472_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:38:51.54 -16:39:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.719 2946923198052242816 099.71522762465 -16.66310880480 14.3914 13.7840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143517_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143517_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:37:25.68 -18:25:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.973 2940444806823307264 099.35727548111 -18.41765175531 14.3456 13.7620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143539_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143539_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:32:32.66 -18:34:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.701 2940392030263111680 098.13648373890 -18.57216304273 14.2227 13.4934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143634_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 143634_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:32:04.51 -16:13:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.566 2949959052737044352 098.01884513822 -16.22243206921 14.6683 14.1184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78098_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 78098_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 93932_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 93932_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 95974_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 95974_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 79265_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 79265_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 121787_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 121787_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:29:19.84 -21:01:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.736 2937450488765187840 097.33393704713 -21.02490280879 12.3412 10.8125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09615_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 09615_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:04:57.41 -22:12:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38701_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 38701_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:57:42.40 -19:16:19.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 29739_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 29739_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:59:18.37 -20:13:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79764_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 79764_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 79528_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 79528_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 19830_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 19830_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:01:51.01 -21:06:14.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103634_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 103634_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:29:57.93 -15:48:07.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 29136_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 29136_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 88435_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 88435_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 15796_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 15796_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 82559_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 82559_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:34:26.71 -13:41:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99144_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 99144_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
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Considering the candidate 12240_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 12240_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 06:06:57.63 -21:48:37.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 19790_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 19790_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 05:51:20.00 -20:52:58.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 87222_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062
The candidate 87222_fd_CMa-01-Q2b1x1_2026-04-05_22-11-46_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
