This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR
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 06.1102* 01 23 28.06 +66 56 20.5 13.4 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6102,13.38,0.05,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
target 20260406.1102 13.38CV 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 06.1102* 01 45 04.20 +72 51 30.7 13.1 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AI Cas,2461136.6102,13.09,0.05,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
AI Cas 20260406.1102 13.09CV 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 06.1102* 01 23 55.60 +66 08 48.3 13.4 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1280,2461136.6102,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1280 20260406.1102 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1102* 01 25 11.67 +65 23 25.0 14.3 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J012511.05+652318.8,2461136.6102,14.30,0.05,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 J012511.05+652318.8 20260406.1102 14.30CV 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 06.1102* 02 43 51.08 +68 52 12.8 13.7 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 385925,2461136.6102,13.65,0.05,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 385925 20260406.1102 13.65CV 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 06.1102* 01 26 32.11 +67 02 56.8 13.0 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0126315+670254,2461136.6102,12.96,0.05,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 J0126315+670254 20260406.1102 12.96CV 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 06.1102* 01 40 48.88 +72 23 49.6 13.7 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014048.99+722346.2,2461136.6102,13.68,0.05,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
ASASSN-V J014048.99+722346.2 20260406.1102 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 06.1102* 03 28 19.59 +70 56 59.7 13.3 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0328205+705703,2461136.6102,13.28,0.05,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
NSVS J0328205+705703 20260406.1102 13.28CV 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 06.1102* 01 29 50.48 +67 02 52.3 13.0 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6102,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1102 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.1102* 01 37 21.58 +68 00 17.5 13.2 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0137216+680017,2461136.6102,13.21,0.05,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
NSVS J0137216+680017 20260406.1102 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 06.1102* 01 30 02.72 +66 52 45.0 13.3 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.6102,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.1102 13.32CV 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 06.1102* 01 32 58.98 +67 48 55.3 12.6 U Cas 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0906 Cas,2461136.6102,12.55,0.05,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
V0906 Cas 20260406.1102 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.58401343 09.01.2026 02:00:48.760 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461049.58401343 09.01.2026 02:00:48.760 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461136.61053442 06.04.2026 02:39:00.174 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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): 14164
Objects passed selection criteria: 14142
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 12494
Average stars matched: 11990 (95.9661 %)
Memory usage VmPeak: 119188 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 21:52:06 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: 2461049.58401343 09.01.2026 02:00:48.760 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
First image: 2461049.58401343 09.01.2026 02:00:48.760 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Last image: 2461136.61053442 06.04.2026 02:39:00.174 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 121
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 52 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): 105561
Objects passed selection criteria: 105316
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 90717.5
Average stars matched: 86756 (95.6331 %)
Memory usage VmPeak: 1886876 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 5 21:54:28 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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
SExtractor catalog cache: saved Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.60994863
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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
Saving wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits to local_wcs_cache/
'wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits' -> 'local_wcs_cache/wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits'
wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
Saving wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits to local_wcs_cache/
'wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits' -> 'local_wcs_cache/wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits'
wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits exists and is non-empty
Saving wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits to local_wcs_cache/
'wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits'
wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.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 02:24:10.600 +69:59:22.54
Second-epoch image center 02:23:58.368 +70:00:09.03
Angular distance between the image centers 0.0217 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 02:24:10.600 +69:59:22.54
Second-epoch image center 02:23:57.708 +70:00:52.35
Angular distance between the image centers 0.0310 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 02:23:58.368 +70:00:09.03
Second-epoch second image center 02:23:57.708 +70:00:52.35
Angular distance between the image centers 0.01207 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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.UxhoS4sBH8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.TtgVG9O3FO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits &> /tmp/tmp.B5CKHv8E6c
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits &> /tmp/tmp.nNIt6KIrLH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat' -> 'wcsmag.cat'
Read 17130 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 8.7395 to 64.5322 deg, Dec +62.8434 to +75.4744 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 8.7395 to 64.5322 deg, Dec 62.8434 to 75.4744 deg
Loaded 15575 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): 7653 out of 8334 total matches.
Matched with Tycho-2 8334 out of 17130 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.962036
a=0.000000 b=1.000000 c=22.962036
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
2.1 pix Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
2.5 pix fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
2.5 pix fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.4 mag. Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
15.4 mag. Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
14.9 mag. fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
14.9 mag. fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (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.UxhoS4sBH8 (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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1459, passed=17130
Got 17130 stars (including 15650 good ones) from the SExtractor catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 17130 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 16121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 16121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 16121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.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.TtgVG9O3FO (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/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1446, passed=17209
Got 17209 stars (including 15733 good ones) from the SExtractor catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 17209 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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 16195 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 16192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 16192 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.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.B5CKHv8E6c (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1090, passed=13142
Got 13142 stars (including 12036 good ones) from the SExtractor catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 13142 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 12765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 12767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 12767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits -region wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.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.nNIt6KIrLH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1126, passed=13140
Got 13140 stars (including 12006 good ones) from the SExtractor catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 13140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 12793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 12796 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 12796 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 963 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits -region wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits'
Saving fully-calibrated image wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits'
Saving fully-calibrated image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits'
Saving fully-calibrated image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits'
Preparing the HTML report for the field Cas-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21841.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21492_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21492_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:52:56.59 +67:56:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21671_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21671_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:15:21.71 +69:09:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.495 541207493237742336 048.84062426814 +69.15540190737 12.0588 11.4949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21712_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21712_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:30:40.14 +70:50:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.605 545262762700335232 037.66751410209 +70.84083842280 11.9601 11.4601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21716_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21716_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:51:29.50 +69:48:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.975 541826896239859584 042.87274454983 +69.80043081045 11.9797 11.3944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21785_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21785_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:27:06.72 +69:12:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.210 493126468230985856 051.77848527169 +69.21503848792 12.2574 11.6044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21790_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21790_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:55:58.96 +69:31:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21841_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 21841_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:27:08.76 +72:26:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.556 546252636700392192 036.78689208352 +72.44743258797 12.2002 11.6446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08506_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 08506_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:42:31.41 +70:25:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11992_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 11992_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:18:21.48 +67:56:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06999_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 06999_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:45:09.03 +71:19:15.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cas-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
SExtractor catalog cache: saved Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat to cache
SExtractor catalog cache: saved Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Creating symlink local_wcs_cache/wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits exists and is non-empty
wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits exists and is non-empty
wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits exists and is non-empty
wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.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 02:24:10.600 +69:59:22.54
Second-epoch image center 02:23:58.368 +70:00:09.03
Angular distance between the image centers 0.0217 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 02:24:10.600 +69:59:22.54
Second-epoch image center 02:23:57.708 +70:00:52.35
Angular distance between the image centers 0.0310 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 02:23:58.368 +70:00:09.03
Second-epoch second image center 02:23:57.708 +70:00:52.35
Angular distance between the image centers 0.01207 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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits &> /tmp/tmp.4v4OxyEIPc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits &> /tmp/tmp.Nhzn5IwHUG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits &> /tmp/tmp.MA7MkW6s1S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits &> /tmp/tmp.K7OGEaFpdT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
Found non-empty wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits and wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
The reference image (wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits) and catalog (wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat) found
'wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat' -> 'wcsmag.cat'
Read 130258 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 8.6566 to 64.6850 deg, Dec +62.8434 to +75.4826 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 8.6566 to 64.6850 deg, Dec 62.8434 to 75.4826 deg
Loaded 15630 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): 6540 out of 8433 total matches.
Matched with Tycho-2 8433 out of 130258 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.833708
a=0.000000 b=1.000000 c=22.833708
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.59
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.59
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 77 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
1.9 pix Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
2.3 pix fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
2.3 pix fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.6 mag. Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
15.6 mag. Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
15.0 mag. fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
15.0 mag. fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.4v4OxyEIPc (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/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits' -> 'wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WCS_IMAGE_NAME=wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WCS-calibrated image found: wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Checking if the catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits alredy exist and is non-empty...
Catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
WCS catalog name: wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=11648, passed=130231
Got 130231 stars (including 118319 good ones) from the SExtractor catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat
util/solve_plate_with_UCAC5 got 130231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 125956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 125958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 125956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits -region wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.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.Nhzn5IwHUG (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/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits' -> 'wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WCS_IMAGE_NAME=wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WCS-calibrated image found: wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
Checking if the catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits alredy exist and is non-empty...
Catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat corresponding to the image wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
WCS catalog name: wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=11687, passed=129707
Got 129707 stars (including 117743 good ones) from the SExtractor catalog wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat
util/solve_plate_with_UCAC5 got 129707 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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 124911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 124912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 124911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits -region wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.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.MA7MkW6s1S (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=8098, passed=80773
Got 80773 stars (including 72560 good ones) from the SExtractor catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 80773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 79068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 79068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
WARNING: Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 79068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits -region wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.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.K7OGEaFpdT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=8039, passed=81103
Got 81103 stars (including 72955 good ones) from the SExtractor catalog wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 81103 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 79651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 79651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 79631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 965 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits -region wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.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_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_Cas-01-Q2b1x1_2026-01-08_20-00-48_20.00sec_-15.00C_LIGHT_0022.fits
Saving fully-calibrated image wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_Cas-01-Q2b1x1_2026-01-08_20-01-43_20.00sec_-15.00C_LIGHT_0023.fits
Saving fully-calibrated image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-38-09_20.00sec_-4.90C_LIGHT_0032.fits
Saving fully-calibrated image wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-05_CI_Cas-01-Q2b1x1_213941_TTUQ2b1x1_8598_v3ehyvcR/wcs_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033.fits
Preparing the HTML report for the field Cas-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out140824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out150088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out150030.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out108416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out150084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77418.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 7s
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Considering the candidate 150030_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150030_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:46:38.43 +65:47:02.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)
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Considering the candidate 150033_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150033_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:36:37.55 +66:18:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.991 519351916500020480 024.15601080148 +66.29995812407 13.8099 12.6335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150034_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150034_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:18:47.33 +67:19:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.904 520308491614401408 034.69756911495 +67.32490338800 14.0417 12.9074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150041_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150041_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:49:48.53 +71:18:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150042_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150042_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 150052_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150052_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 150054_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150054_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:13:00.12 +70:05:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.315 533195008410882688 018.24861500894 +70.09904211572 13.3602 12.2488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150055_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150055_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:00:12.46 +71:48:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.470 542652144139578624 045.05266312538 +71.81264092128 14.2574 13.5000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150059_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150059_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:55:47.17 +72:59:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.387 543522652408646144 058.94784515590 +72.98480752967 14.2081 13.6165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150060_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150060_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:52:28.41 +72:49:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.915 534501571819927296 028.12009513495 +72.82257433772 14.1244 13.5325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150064_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150064_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:26:20.71 +65:05:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.008 513230179357098240 021.58569622246 +65.08751925346 13.2540 12.5932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150067_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150067_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:30:00.88 +66:58:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150072_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150072_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:42:16.12 +71:43:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 0.781 543333158451198592 055.56781157803 +71.72750445166 13.7860 13.0138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150079_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150079_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:26:28.76 +65:24:40.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 150081_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150081_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:27:15.88 +71:20:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.831 534091144747078784 021.81832979649 +71.34440389851 13.7488 13.2025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150084_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 150084_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 150088_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150088_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:28:45.61 +65:08:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.071 513239727061855872 022.19263997505 +65.13534754637 12.5231 11.9617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 150090_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150090_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:41:03.09 +65:43:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150094_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150094_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:45:01.89 +72:51:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150686_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 150686_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:52:56.66 +67:56:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151310_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 151310_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:25:30.22 +65:28:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151716_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 151716_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:17:23.98 +70:32:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151874_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 151874_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 151935_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 151935_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:25:59.31 +68:05:41.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151996_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 151996_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:27:50.09 +72:09:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152139_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152139_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:27:51.17 +72:09:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152194_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152194_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:02:58.39 +71:16:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152207_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152207_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:42:36.20 +70:35:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152269_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152269_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:38:10.29 +73:03:32.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152335_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152335_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:34:40.91 +65:46:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152366_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152366_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:22:43.03 +70:20:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152506_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 152506_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 152579_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152579_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:03:26.60 +73:51:57.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 152789_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152789_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:58:49.90 +70:45:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152825_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152825_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:10:30.52 +68:41:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152852_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 152852_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:32:13.58 +71:43:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153211_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153211_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:51:47.85 +66:37:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153277_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153277_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:54:10.81 +69:12:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153306_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153306_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:34:34.48 +70:16:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.729 533772801770425600 023.64319710988 +70.27995739426 13.5815 11.4111 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153385_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153385_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:42:20.17 +69:05:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153456_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153456_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:10:04.56 +73:08:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153458_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153458_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:07:36.43 +67:35:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 4.188 540585272736766592 046.89898643742 +67.58859690992 14.2508 13.5248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153598_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153598_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:08:19.64 +69:18:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153739_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153739_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:25:02.60 +66:49:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 2.194 517231714482697728 036.26166103687 +66.82890150184 13.9208 13.0537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153782_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153782_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:54:47.24 +72:06:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153807_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153807_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:31:21.70 +69:26:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153837_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 153837_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:24:30.84 +65:46:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 4.669 525294501971438208 021.12605118691 +65.76695793268 13.2531 11.8740 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154128_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154128_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:12:12.27 +69:15:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.784 541132176691800704 048.05237031227 +69.25078128048 13.7066 12.5862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154250_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154250_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:22:44.62 +68:25:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154258_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154258_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:34:03.22 +70:38:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154389_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154389_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:32:02.48 +65:11:21.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)
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Considering the candidate 154524_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154524_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:23:29.05 +73:28:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 2.723 546917493342441728 035.87332331514 +73.47216635717 14.4329 13.7065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154549_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 154549_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 154776_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154776_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:54:15.25 +70:24:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.281 521828635158622208 028.56260324188 +70.40411035158 13.0491 11.5367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154777_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154777_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:53:21.84 +68:46:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 0.747 541700001429993344 043.34152145700 +68.77250305302 12.5106 10.9538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154831_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154831_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:13:51.88 +65:35:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.198 492060697867936256 048.46624377264 +65.59023296345 14.5152 13.4923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154922_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154922_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:04:52.45 +69:16:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.735 541355751210749568 046.21731738764 +69.27398904797 15.0350 14.2637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154960_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 154960_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:21:32.57 +70:37:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.638 542982105004647040 050.38522745894 +70.62968868178 14.7967 13.9945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142474_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 142474_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:55:59.04 +69:31:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123948_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 123948_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:19:25.78 +68:04:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126042_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 126042_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:33:20.67 +68:28:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122370_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 122370_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:18:21.51 +67:56:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77418_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 77418_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 110559_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 110559_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 37203_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 37203_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 34758_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 34758_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 110394_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 110394_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 95738_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 95738_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:35:39.31 +66:28:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.547 519427026890150400 023.91250970025 +66.47660253898 12.9732 11.7643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121393_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 121393_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 113983_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 113983_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 02:15:15.44 +68:44:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96871_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 96871_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:25:27.22 +65:52:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108416_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 108416_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 51772_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 51772_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:45:09.13 +71:19:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140824_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 140824_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 03:30:50.43 +68:46:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 119631_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
Preparing report for the candidate 119631_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
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Considering the candidate 63786_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 63786_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
**** FOUND 01:42:31.37 +70:25:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53046_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033
The candidate 53046_fd_Cas-01-Q2b1x1_2026-04-05_21-39-00_20.00sec_-5.00C_LIGHT_0033 did not pass the final checks
