This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl
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!
TCP 2026 04 10.1516* 05 36 16.57 +21 16 07.6 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 11.59CV 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!
TCP 2026 04 10.1516* 05 14 02.46 +20 34 08.0 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6516,13.68,0.05,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 20260410.1516 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 18 37.12 +19 03 20.3 13.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3401634512413664256,2461140.6516,13.43,0.05,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 3401634512413664256 20260410.1516 13.43CV 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!
TCP 2026 04 10.1516* 05 28 02.50 +26 14 05.2 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 12.38CV 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!
TCP 2026 04 10.1516* 05 43 27.70 +19 15 31.7 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 12.78CV 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!
TCP 2026 04 10.1516* 05 32 56.41 +18 49 37.2 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 30 38.52 +22 15 29.8 13.1 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 13.11CV 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!
TCP 2026 04 10.1516* 05 27 24.92 +23 07 31.6 13.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6516,13.52,0.05,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 20260410.1516 13.52CV 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!
TCP 2026 04 10.1516* 05 47 24.15 +22 03 55.3 13.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.8493+22.0758,2461140.6516,13.89,0.05,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
ATO J086.8493+22.0758 20260410.1516 13.89CV 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!
TCP 2026 04 10.1516* 05 49 54.93 +20 33 37.9 13.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.4808+20.5600,2461140.6516,13.84,0.05,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
ATO J087.4808+20.5600 20260410.1516 13.84CV 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!
TCP 2026 04 10.1516* 05 43 19.96 +19 14 37.1 13.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 13.79CV 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!
TCP 2026 04 10.1516* 05 36 47.16 +23 22 45.8 14.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,14.16,0.05,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
VARIABLE_NAME 20260410.1516 14.16CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 14 38.10 +20 37 22.1 12.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051437.90+203721.4,2461140.6516,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J051437.90+203721.4 20260410.1516 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 22 03.39 +23 24 09.4 12.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J052203.20+232411.4,2461140.6516,12.60,0.05,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 J052203.20+232411.4 20260410.1516 12.60CV 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!
TCP 2026 04 10.1516* 05 22 25.41 +22 44 24.7 12.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0522251+224426,2461140.6516,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0522251+224426 20260410.1516 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 38 32.56 +25 00 04.5 8.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GP Tau,2461140.6516,8.28,0.05,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
GP Tau 20260410.1516 8.28CV 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!
TCP 2026 04 10.1516* 05 19 02.22 +24 45 46.9 9.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 1919,2461140.6516,9.21,0.05,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
NSV 1919 20260410.1516 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!
TCP 2026 04 10.1516* 05 18 59.04 +23 30 29.7 10.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,10.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 10.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 16 40.56 +24 26 20.6 12.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0516403+242624,2461140.6516,12.71,0.05,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 J0516403+242624 20260410.1516 12.71CV 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!
TCP 2026 04 10.1516* 05 41 01.25 +20 16 27.1 13.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.6516,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.1516 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 20 59.06 +25 08 37.4 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J052059+2508.7,2461140.6516,11.63,0.05,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 J052059+2508.7 20260410.1516 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 31 41.32 +18 35 28.9 10.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J053141+1835.5,2461140.6516,10.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J053141+1835.5 20260410.1516 10.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 24 42.96 +24 38 08.4 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J052442.92+243812.6,2461140.6516,13.62,0.05,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
ZTF J052442.92+243812.6 20260410.1516 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 33 52.68 +23 22 00.2 11.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J053353+2322.0,2461140.6516,11.18,0.05,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 J053353+2322.0 20260410.1516 11.18CV 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!
TCP 2026 04 10.1516* 05 29 02.02 +21 26 46.8 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.2577+21.4382,2461140.6516,13.71,0.05,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 J082.2577+21.4382 20260410.1516 13.71CV 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!
TCP 2026 04 10.1516* 05 21 12.59 +19 30 28.6 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 9563165,2461140.6516,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 9563165 20260410.1516 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 39 15.36 +20 28 55.5 13.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0539157+202855,2461140.6516,12.98,0.05,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 J0539157+202855 20260410.1516 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1516* 05 37 21.40 +17 53 27.9 12.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053721.47+175328.1,2461140.6516,12.85,0.05,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
ASASSN-V J053721.47+175328.1 20260410.1516 12.85CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461140.65188751 10.04.2026 03:38:33.081 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 5 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): 19926
Objects passed selection criteria: 19844
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 14909.5
Average stars matched: 13105.8 (87.902 %)
Memory usage VmPeak: 121972 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:42:04 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461140.65188751 10.04.2026 03:38:33.081 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 208
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 50 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): 139061
Objects passed selection criteria: 138702
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 102463
Average stars matched: 91332.2 (89.1368 %)
Memory usage VmPeak: 1954288 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:44:33 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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: 2461140.65126227
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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits'
wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:31.785 +22:00:04.52
Angular distance between the image centers 0.0470 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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:34.508 +21:59:45.67
Angular distance between the image centers 0.0577 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 05:32:31.785 +22:00:04.52
Second-epoch second image center 05:32:34.508 +21:59:45.67
Angular distance between the image centers 0.01175 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.Iuxyzehi7m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.fLdwkVTe5F
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits &> /tmp/tmp.PnxguEhmmY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits &> /tmp/tmp.KlunwboXxH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat' -> 'wcsmag.cat'
Read 23525 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.1682 to 91.6910 deg, Dec +16.3328 to +27.3474 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 74.1682 to 91.6910 deg, Dec 16.3328 to 27.3474 deg
Loaded 12326 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): 9058 out of 10254 total matches.
Matched with Tycho-2 10254 out of 23525 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.945337
a=0.000000 b=1.000000 c=22.945337
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.3 pix Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.3 mag. Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
14.7 mag. fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
14.7 mag. fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Iuxyzehi7m (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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2582, passed=23525
Got 23525 stars (including 20915 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 23525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 22051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 22047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 22047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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.fLdwkVTe5F (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/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2595, passed=23514
Got 23514 stars (including 20891 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 23514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 22179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 22181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 22181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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.PnxguEhmmY (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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1351, passed=16009
Got 16009 stars (including 14648 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 16009 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 15334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 15331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 15332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.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.KlunwboXxH (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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1345, passed=16002
Got 16002 stars (including 14647 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 16002 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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 15341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 15339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 15339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out34162.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34162_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 34162_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34346_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 34346_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:16:29.08 +20:02:21.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34435_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 34435_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:34:26.32 +20:22:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04457_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 04457_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:18:00.42 +18:21:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30860_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 30860_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:56.36 +17:54:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04007_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 04007_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:33:35.18 +18:20:57.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:36:16.57 +21:16:07.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:31.785 +22:00:04.52
Angular distance between the image centers 0.0470 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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:34.508 +21:59:45.67
Angular distance between the image centers 0.0577 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 05:32:31.785 +22:00:04.52
Second-epoch second image center 05:32:34.508 +21:59:45.67
Angular distance between the image centers 0.01175 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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.JRm7XPlfkz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.4jApiV1Wwu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits &> /tmp/tmp.RBsGRYmnnk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits &> /tmp/tmp.Dbc5RPwr0f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat' -> 'wcsmag.cat'
Read 163644 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.1103 to 91.6919 deg, Dec +16.3196 to +27.3524 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 74.1103 to 91.6919 deg, Dec 16.3196 to 27.3524 deg
Loaded 12375 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): 7170 out of 10499 total matches.
Matched with Tycho-2 10499 out of 163644 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.769457
a=0.000000 b=1.000000 c=22.769457
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 177 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.0 pix Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.5 mag. Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
14.7 mag. fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
14.7 mag. fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.JRm7XPlfkz (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/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=21410, passed=163589
Got 163589 stars (including 141908 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 163589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 154538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 154540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 154537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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.4jApiV1Wwu (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/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=21418, passed=163772
Got 163772 stars (including 142086 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 163772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 154756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 154755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 154755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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.RBsGRYmnnk (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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=10227, passed=90711
Got 90711 stars (including 80377 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 90711 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 86211 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 86212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 86212 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 929 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.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.Dbc5RPwr0f (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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=10452, passed=91092
Got 91092 stars (including 80563 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 91092 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 86300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 86297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 86296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 923 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits -region wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-37-39_20.00sec_-5.00C_LIGHT_0012.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.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_2026-04-09_CI_Tau-04-Q2b1x1_223927_TTUQ2b1x1_15839_FfPIcnOl/wcs_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out174400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out207049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out207062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out207465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out207468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out215351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out206626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out207496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98863.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 25s
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: 14s
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Considering the candidate 185126_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185126_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 185130_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185130_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 185136_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185136_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:51:06.76 +23:22:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185148_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185148_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:07.88 +25:43:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185150_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 185150_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 185167_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185167_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:22.67 +26:17:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185168_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 185168_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 185176_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185176_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:59.74 +20:34:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185177_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185177_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:48.97 +19:18:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.226 3399264029767582080 086.45377721237 +19.30320460477 14.0817 13.5702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185184_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185184_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:57.11 +21:51:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185186_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185186_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:30.04 +20:34:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.139 3399868589364669696 087.62535293651 +20.56912526007 12.6473 12.2009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185188_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185188_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:08.79 +21:32:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185189_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185189_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:04.22 +24:54:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185190_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185190_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:51:04.90 +22:35:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 185192_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 185192_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:48.96 +20:33:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188438_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 188438_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:16.69 +21:16:08.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 190149_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 190149_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:56.09 +22:38:54.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191062_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 191062_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:35.70 +25:17:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191579_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 191579_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:35.67 +23:46:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192057_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 192057_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:21.59 +18:36:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192624_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 192624_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 192761_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 192761_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:43:00.22 +18:59:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192771_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 192771_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:08.56 +21:18:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193735_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 193735_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:50.19 +21:18:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194125_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 194125_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:51:30.82 +18:25:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194280_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 194280_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:42:46.93 +21:22:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194344_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 194344_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:43:08.85 +20:03:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194498_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 194498_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 195787_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 195787_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:52.29 +21:18:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195806_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 195806_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 195845_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 195845_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:20:11.73 +19:34:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195891_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 195891_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:39:11.35 +19:48:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196066_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196066_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:03.93 +24:38:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196069_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196069_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:02.92 +20:17:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196139_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196139_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:31:10.89 +20:10:03.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196272_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196272_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:32.51 +23:52:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196610_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196610_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:40.08 +20:11:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196746_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196746_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:42.20 +23:00:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196775_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 196775_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:49.40 +18:34:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197016_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 197016_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:21.77 +21:11:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197050_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 197050_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:19:43.90 +26:10:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197174_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 197174_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:32:03.06 +18:33:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197441_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 197441_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:29.09 +18:44:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198426_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 198426_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 198679_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198679_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:50.95 +20:15:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198700_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198700_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:07.68 +19:32:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198762_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198762_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:02.36 +24:22:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198855_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198855_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:10.46 +20:05:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198856_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198856_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:35:18.98 +21:12:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198861_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198861_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:54.89 +19:05:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198931_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198931_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:20.15 +24:24:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198937_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 198937_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:28:32.07 +22:45:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199321_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 199321_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:05.60 +23:11:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199390_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 199390_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:39:57.89 +24:13:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199742_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 199742_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:53.42 +18:32:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200444_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 200444_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:13.55 +25:22:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200741_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 200741_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:25.07 +25:30:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201710_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 201710_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:11.93 +19:49:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201772_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 201772_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:39:27.48 +21:47:31.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201783_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 201783_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:56.61 +22:39:44.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201793_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 201793_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:27.58 +18:02:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 201886_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 201886_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:11.43 +25:40:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202040_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 202040_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:39:37.12 +25:18:47.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202210_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 202210_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:16:46.45 +20:08:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202290_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 202290_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:32:41.26 +20:56:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202794_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 202794_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:18:29.69 +21:46:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202914_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 202914_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:39.77 +21:50:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.364 3424218996645780864 087.41610749636 +21.84120891313 13.7698 12.9350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203267_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203267_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:06.91 +24:22:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203422_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203422_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:48.01 +21:18:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203465_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203465_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:37.21 +23:37:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203496_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203496_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:24:12.98 +20:07:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203661_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203661_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:06.30 +24:25:28.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203707_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203707_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:40.33 +18:15:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203711_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203711_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:20:20.26 +25:09:00.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203732_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 203732_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203815_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203815_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:37.79 +19:23:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203877_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203877_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:35:45.43 +21:24:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203937_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 203937_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:08.06 +19:33:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204066_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204066_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:43:10.29 +18:50:07.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204148_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204148_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:27:27.48 +18:28:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204238_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204238_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:21.84 +24:21:24.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204279_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204279_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:43.96 +24:53:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204418_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204418_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:47:20.96 +23:52:57.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204549_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204549_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:38.51 +25:25:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204618_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204618_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:40.65 +18:53:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204716_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204716_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:23:51.92 +20:00:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204779_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204779_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:14.66 +21:13:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204902_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 204902_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:17:30.48 +20:09:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205431_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205431_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:55.27 +22:57:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205597_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205597_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:41.87 +20:11:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.936 3399750220067616512 086.67410227652 +20.18712420744 14.0452 13.4817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205652_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205652_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:20.93 +24:21:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205676_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205676_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:49.61 +25:55:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205795_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205795_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:08.40 +20:02:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205835_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205835_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:12.58 +20:42:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205848_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205848_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:51:37.42 +19:17:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205865_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 205865_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:34:57.03 +25:53:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205968_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 205968_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206066_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206066_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:20.03 +25:31:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206101_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206101_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:36.32 +19:12:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206403_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206403_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:34:30.07 +21:59:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206555_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206555_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:42:31.45 +18:39:28.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206626_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 206626_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206762_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206762_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:35:34.61 +21:24:28.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206788_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206788_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:54.25 +19:27:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206811_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206811_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:38:09.69 +18:34:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 206852_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 206852_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:37:08.21 +22:06:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207049_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207049_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:41:17.13 +22:13:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.297 3403381842549049728 085.32175993919 +22.22361273138 13.8148 13.3188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207062_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207062_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:36.61 +20:18:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.462 3399945353316900096 086.65348669951 +20.30703977616 13.8208 12.9187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207465_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207465_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:25.67 +20:26:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.494 3399818840760563456 087.60623810338 +20.43990596434 14.3437 13.8470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 207468_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207468_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:44.74 +18:59:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.431 3398495853394295296 087.18681895650 +18.98347625737 13.6383 12.7525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 207496_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 207496_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 207565_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207565_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:39:30.95 +20:47:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207576_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207576_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:37:56.32 +22:27:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207820_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207820_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:33:24.44 +18:32:31.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 207930_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207930_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:56.70 +21:39:38.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207979_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 207979_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:26.35 +23:40:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208032_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 208032_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:40:20.57 +22:11:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208922_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 208922_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:45:11.64 +18:12:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209069_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 209069_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:42:23.85 +23:10:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209379_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 209379_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:37:31.13 +19:46:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209381_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 209381_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:55.14 +24:07:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209482_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 209482_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:44.29 +18:15:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209777_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 209777_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:50.79 +22:02:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210113_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 210113_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:58.14 +20:38:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210441_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 210441_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:57.85 +21:39:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210792_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 210792_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:38:57.01 +21:39:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211237_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211237_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:42:08.90 +18:54:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211426_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211426_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:44:37.61 +20:42:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211503_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211503_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:24.17 +18:21:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.690 3398393044759599104 087.10108608296 +18.35108063095 13.8353 12.9430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211591_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211591_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:09.94 +23:51:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211605_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211605_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:36:24.93 +22:00:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211750_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211750_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:43:45.85 +19:03:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211815_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211815_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:05.12 +22:46:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.759 3427521826496062464 086.52072455780 +22.77549415347 14.4611 13.7981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211941_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 211941_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:20.74 +25:32:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212341_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 212341_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 212669_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 212669_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:31.10 +23:26:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212677_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 212677_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:50:38.35 +18:55:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 3.588 3398440121899185152 087.66079331771 +18.91944779581 14.5546 14.0329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212679_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 212679_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:42:30.41 +22:05:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215032_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 215032_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:48:06.96 +21:23:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.944 3400159826804136832 087.02918733309 +21.39006659848 14.4090 13.4886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215194_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 215194_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:39:39.34 +23:43:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.693 3404429741552884480 084.91425487233 +23.72668719391 13.6396 12.1902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215257_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 215257_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:31.62 +20:44:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.714 3399887113560266624 087.38190586698 +20.73934207632 14.6652 14.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 215351_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 215351_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:49:02.44 +23:10:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 3.550 3427375179132723968 087.25939783455 +23.17499324535 14.8234 14.0276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 132765_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 132765_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:28:44.53 +24:57:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65702_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 65702_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 109160_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 109160_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 98863_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 98863_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 126512_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 126512_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 147078_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 147078_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:18:56.74 +23:52:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174837_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 174837_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:51:41.62 +23:34:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133391_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 133391_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 111963_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 111963_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 27303_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 27303_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:33:35.19 +18:20:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59246_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 59246_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:34:26.35 +20:22:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62296_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 62296_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:32:32.91 +20:37:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138031_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 138031_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 18025_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 18025_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:46:56.36 +17:54:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56165_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 56165_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 128052_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 128052_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 134975_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 134975_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:42:11.85 +24:53:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31993_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 31993_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 136732_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 136732_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 107372_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 107372_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 140655_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 140655_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:33:29.11 +24:26:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56342_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 56342_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:16:29.10 +20:02:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76383_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 76383_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 16885_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 16885_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:37:44.00 +17:45:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81521_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 81521_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:15:53.65 +21:35:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112873_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 112873_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:17:14.06 +23:35:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46547_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 46547_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 59475_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 59475_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 131291_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 131291_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:30:04.34 +25:01:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18303_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
Preparing report for the candidate 18303_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
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Considering the candidate 77701_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 77701_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:17:28.66 +21:23:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105052_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 105052_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:24:49.56 +23:06:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29777_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 29777_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:18:00.49 +18:21:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174400_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 174400_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
**** FOUND 05:40:56.23 +21:25:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.487 3403127408685617664 085.23498190297 +21.42691317647 11.6038 9.9142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 146579_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013
The candidate 146579_fd_Tau-04-Q2b1x1_2026-04-09_22-38-33_20.00sec_-4.90C_LIGHT_0013 did not pass the final checks
