This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 49 29.37 +45 29 53.6 11.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 1338,2461140.6439,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 1338 20260410.1439 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 10 45.34 +49 13 41.1 11.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0310453+491342,2461140.6439,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0310453+491342 20260410.1439 11.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 10 23.62 +45 49 03.2 12.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J047.6139+45.8175,2461140.6439,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J047.6139+45.8175 20260410.1439 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 23 20.83 +41 42 38.0 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6439,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1439 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 43 41.17 +42 35 58.1 13.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6439,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1439 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 23 06.39 +46 13 21.1 10.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J032306.27+461321.5,2461140.6439,10.37,0.05,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
ASASSN-V J032306.27+461321.5 20260410.1439 10.37CV 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 10.1439* 04 00 20.61 +42 03 01.7 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0400211+420256,2461140.6439,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0400211+420256 20260410.1439 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 37 19.70 +48 24 21.0 13.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J033720.05+482424.8,2461140.6439,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J033720.05+482424.8 20260410.1439 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 16 39.74 +49 48 03.9 11.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0316406+494818,2461140.6439,11.93,0.05,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 J0316406+494818 20260410.1439 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 31 37.25 +47 45 29.1 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4123600,2461140.6439,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4123600 20260410.1439 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 11 57.88 +46 33 41.4 12.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J031157.50+463343.9,2461140.6439,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J031157.50+463343.9 20260410.1439 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 29 49.77 +46 09 57.4 12.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0329497+460959,2461140.6439,12.76,0.05,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 J0329497+460959 20260410.1439 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 23 27.97 +47 36 48.4 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J032327.83+473649.4,2461140.6439,13.21,0.05,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
ZTF J032327.83+473649.4 20260410.1439 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 40 37.56 +50 02 14.7 13.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4132016,2461140.6439,13.47,0.05,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 4132016 20260410.1439 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 21 49.66 +48 15 50.0 11.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J032149.46+481552.1,2461140.6439,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J032149.46+481552.1 20260410.1439 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 29 38.97 +46 48 37.4 13.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J032938.97+464837.4,2461140.6439,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J032938.97+464837.4 20260410.1439 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 33 37.03 +50 08 09.3 12.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0333370+500811,2461140.6439,12.28,0.05,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 J0333370+500811 20260410.1439 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 26 05.73 +47 54 22.5 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 4118614,2461140.6439,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 4118614 20260410.1439 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 12 47.21 +48 27 06.5 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J031246.90+482709.1,2461140.6439,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J031246.90+482709.1 20260410.1439 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.1439* 03 15 14.85 +46 34 51.2 7.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AA Per,2461140.6439,7.93,0.05,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
AA Per 20260410.1439 7.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.59394793 18.01.2026 02:15:07.101 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
First image: 2461058.59394793 18.01.2026 02:15:07.101 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Last image: 2461140.64419542 10.04.2026 03:27:28.484 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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): 20925
Objects passed selection criteria: 20817
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 14724.8
Average stars matched: 13493.8 (91.6399 %)
Memory usage VmPeak: 123952 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:29:42 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.59394793 18.01.2026 02:15:07.101 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
First image: 2461058.59394793 18.01.2026 02:15:07.101 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Last image: 2461140.64419542 10.04.2026 03:27:28.484 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 131
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 39 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): 149084
Objects passed selection criteria: 148621
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 104523
Average stars matched: 95713.5 (91.5715 %)
Memory usage VmPeak: 2034548 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 22:32:21 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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461140.64353569
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
Saving wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits to local_wcs_cache/
'wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits' -> 'local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits'
wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits exists and is non-empty
Saving wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits to local_wcs_cache/
'wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits' -> 'local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits'
wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits exists and is non-empty
Saving wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits to local_wcs_cache/
'wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits'
wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits exists and is non-empty
Saving wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits to local_wcs_cache/
'wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.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 03:35:57.897 +45:59:42.08
Second-epoch image center 03:35:58.814 +45:59:26.90
Angular distance between the image centers 0.0050 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 03:35:57.897 +45:59:42.08
Second-epoch image center 03:36:01.624 +45:59:02.48
Angular distance between the image centers 0.0154 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 03:35:58.814 +45:59:26.90
Second-epoch second image center 03:36:01.624 +45:59:02.48
Angular distance between the image centers 0.01059 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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.XEnzSCVV80
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits &> /tmp/tmp.LUVSQn5PGc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits &> /tmp/tmp.mqhpGg128P
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits &> /tmp/tmp.55weQbLIvm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits and wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits and wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
Found non-empty wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits and wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
The reference image (wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits) and catalog (wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat) found
'wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat' -> 'wcsmag.cat'
Read 24504 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2404 to 65.8858 deg, Dec +39.8272 to +51.4043 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 41.2404 to 65.8858 deg, Dec 39.8272 to 51.4043 deg
Loaded 12575 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): 8360 out of 9383 total matches.
Matched with Tycho-2 9383 out of 24504 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.926308
a=0.000000 b=1.000000 c=22.926308
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
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 Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
2.1 pix Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
2.9 pix fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
2.9 pix fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Limiting magnitude estimates:
15.3 mag. Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
15.3 mag. Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
14.3 mag. fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
14.3 mag. fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.XEnzSCVV80 (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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2470, passed=24504
Got 24504 stars (including 22005 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 24504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 23738 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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 23739 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 23739 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.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.LUVSQn5PGc (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/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2491, passed=24561
Got 24561 stars (including 22034 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat
util/solve_plate_with_UCAC5 got 24561 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 23683 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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 23682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 23679 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 974 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits -region wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.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.mqhpGg128P (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1033, passed=12529
Got 12529 stars (including 11493 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 12529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 651 to 708 (Dec 40.3 to 51.2)
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...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12163 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits -region wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.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.55weQbLIvm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=946, passed=12459
Got 12459 stars (including 11509 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 12459 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 651 to 708 (Dec 40.3 to 51.2)
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...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 12103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 12102 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits -region wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits'
Saving fully-calibrated image wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits'
Preparing the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out10371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23039.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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
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Considering the candidate 31215_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 31215_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:59:54.63 +48:32:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 0.944 247006081755072896 059.97782728779 +48.53627457762 11.1536 10.1672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33150_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 33150_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:54:56.37 +48:36:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33205_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 33205_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:26:29.78 +47:31:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34191_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 34191_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:13:24.72 +49:46:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10371_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 10371_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 06919_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 06919_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:23:35.27 +43:39:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10985_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 10985_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:24:48.39 +45:27:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23039_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 23039_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 19558_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 19558_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:43:48.18 +49:16:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06768_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 06768_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:12:15.68 +43:20:11.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Per-02-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 ####
03:49:29.37 +45:29:53.6
03:10:45.34 +49:13:41.1
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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Creating symlink local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.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 03:35:57.897 +45:59:42.08
Second-epoch image center 03:35:58.814 +45:59:26.90
Angular distance between the image centers 0.0050 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 03:35:57.897 +45:59:42.08
Second-epoch image center 03:36:01.624 +45:59:02.48
Angular distance between the image centers 0.0154 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 03:35:58.814 +45:59:26.90
Second-epoch second image center 03:36:01.624 +45:59:02.48
Angular distance between the image centers 0.01059 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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.yHQGyX9AlL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits &> /tmp/tmp.MSg6uSEPW8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits &> /tmp/tmp.B8yEkiXuEf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits &> /tmp/tmp.mZWyUTyyNn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits and wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits and wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
Found non-empty wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits and wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
The reference image (wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits) and catalog (wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat) found
'wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat' -> 'wcsmag.cat'
Read 175950 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2237 to 65.8949 deg, Dec +39.7818 to +51.4068 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 41.2237 to 65.8949 deg, Dec 39.7818 to 51.4068 deg
Loaded 12650 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): 6550 out of 9462 total matches.
Matched with Tycho-2 9462 out of 175950 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784720
a=0.000000 b=1.000000 c=22.784720
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 110 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
1.9 pix Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
2.7 pix fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
2.8 pix fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Limiting magnitude estimates:
15.5 mag. Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
15.5 mag. Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
14.4 mag. fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
14.4 mag. fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yHQGyX9AlL (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/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=22504, passed=175909
Got 175909 stars (including 153117 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 175909 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 172522 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 172523 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 172525 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.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.MSg6uSEPW8 (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/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=22668, passed=175587
Got 175587 stars (including 152651 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat
util/solve_plate_with_UCAC5 got 175587 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 172425 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 172428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 172428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits -region wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.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.B8yEkiXuEf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=8189, passed=74993
Got 74993 stars (including 66749 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 74993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 72767 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 72768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 72768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 961 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits -region wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.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.mZWyUTyyNn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=7923, passed=74467
Got 74467 stars (including 66481 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 74467 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 651 to 708 (Dec 40.3 to 51.3)
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...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 72116 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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 72116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 72115 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits -region wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.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_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_Per-02-Q2b1x1_2026-01-17_20-15-07_20.00sec_-15.00C_LIGHT_0027.fits
Saving fully-calibrated image wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_Per-02-Q2b1x1_2026-01-17_20-15-54_20.00sec_-14.90C_LIGHT_0028.fits
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-26-31_20.00sec_-4.90C_LIGHT_0000.fits
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Per-02-Q2b1x1_222824_TTUQ2b1x1_11223_ryKDolXk/wcs_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001.fits
Preparing the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out198747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out214120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out69638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out104083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out144806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96497.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 8s
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Considering the candidate 198744_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198744_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:18:21.64 +47:38:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198747_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198747_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:38:39.71 +42:17:37.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 198751_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198751_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:43:28.19 +48:37:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.373 248664076570550656 055.86820089049 +48.63028235447 13.2480 12.0916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198756_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198756_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:51:59.00 +46:11:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198763_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 198763_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 198766_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 198766_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 198767_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198767_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:13:54.00 +43:50:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198768_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198768_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:47:46.31 +46:39:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198773_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198773_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:51:30.62 +46:15:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198774_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198774_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 04:00:44.87 +49:41:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198775_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198775_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:57:53.33 +43:49:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198777_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 198777_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:59:54.64 +48:32:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 1.082 247006081755072896 059.97782728779 +48.53627457762 11.1536 10.1672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201625_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 201625_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:27:58.89 +49:01:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202027_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 202027_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:13:24.76 +49:46:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202370_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 202370_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 04:00:17.45 +46:48:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202519_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 202519_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:47:09.64 +44:04:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203077_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 203077_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:51:30.09 +45:27:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.825 244171158520339840 057.87567109916 +45.45879120553 11.0795 9.6633 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203163_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 203163_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:53:44.09 +48:40:43.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203402_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 203402_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:30:25.94 +48:06:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204155_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 204155_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:46:04.14 +45:42:23.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204291_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 204291_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:17:57.94 +44:02:07.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204902_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 204902_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:21:50.71 +49:05:42.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 205196_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 205196_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:59:24.03 +49:25:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205256_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 205256_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:47:06.27 +45:08:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 205466_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 205466_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:53:46.76 +48:40:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 206394_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 206394_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:47:46.57 +46:45:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207064_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 207064_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:56:29.63 +44:55:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207102_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 207102_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:56:05.25 +47:51:21.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 207269_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 207269_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:38:22.46 +47:33:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207838_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 207838_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:30:43.48 +48:01:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207888_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 207888_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:31:48.86 +48:45:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208122_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 208122_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:13:55.66 +43:53:17.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 208285_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 208285_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:54:45.78 +47:38:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208348_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 208348_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:33:28.20 +47:56:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208431_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 208431_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:50:34.95 +42:36:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208715_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 208715_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:32:41.00 +44:50:02.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 208810_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 208810_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 04:00:32.58 +42:14:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209617_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 209617_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 209703_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 209703_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:59:26.79 +48:44:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209706_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 209706_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:58:02.40 +48:44:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209803_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 209803_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:12:34.43 +47:44:38.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 210026_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210026_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:37:53.92 +42:35:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 210171_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210171_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:21:50.61 +49:02:22.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 210341_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210341_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:44:45.28 +44:05:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210552_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210552_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 04:00:56.47 +46:40:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210629_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210629_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:31:56.90 +48:33:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210716_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210716_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:45:10.35 +44:45:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210724_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210724_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:51:02.62 +46:15:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 210852_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 210852_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:22:06.20 +42:48:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211048_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211048_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:37:00.70 +43:13:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211058_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211058_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:35:29.00 +42:53:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211202_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211202_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:48:18.79 +47:36:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211240_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211240_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:51:29.33 +47:33:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211577_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211577_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:40:30.12 +49:34:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211749_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211749_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:19:15.57 +50:06:43.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 211761_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211761_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:47:48.51 +46:45:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211774_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211774_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:58:57.56 +43:38:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211811_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211811_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:20:53.80 +44:22:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211980_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 211980_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:26:04.88 +49:46:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212073_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 212073_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:13:28.35 +48:12:24.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212156_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 212156_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:50:13.35 +44:58:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212178_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 212178_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:53:52.65 +48:55:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212215_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 212215_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:52:40.23 +49:07:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212961_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 212961_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:58:05.48 +47:13:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213299_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 213299_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:41:23.10 +44:35:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213455_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 213455_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:40:03.97 +48:56:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213840_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 213840_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:49:08.45 +43:56:27.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 214022_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 214022_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:36:05.32 +49:34:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 214120_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 214120_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 04:00:45.06 +48:14:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 2.207 246799304849522176 060.18712918642 +48.24068608064 14.2197 13.5301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 214324_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 214324_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 04:01:55.07 +48:13:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 215904_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 215904_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:58:07.65 +45:49:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 217613_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 217613_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:48:16.21 +49:14:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96497_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 96497_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 16592_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 16592_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144806_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 144806_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 166947_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 166947_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 121690_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 121690_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 106455_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 106455_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 47465_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 47465_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:15:49.73 +43:25:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92246_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 92246_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 143471_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 143471_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:54:56.36 +48:36:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121005_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 121005_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 108508_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 108508_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:50:56.15 +47:14:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168895_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 168895_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 44626_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 44626_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:37:24.88 +43:39:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142942_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 142942_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 58652_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 58652_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:15:48.05 +44:03:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48064_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 48064_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:12:15.73 +43:20:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118608_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 118608_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:26:29.80 +47:31:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104083_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 104083_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 165931_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 165931_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 69638_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 69638_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:33:30.75 +44:59:55.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 82135_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 82135_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:24:48.40 +45:27:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172947_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 172947_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:10:45.45 +49:13:40.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 174125_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 174125_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:37:08.63 +49:39:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149044_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 149044_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:51:54.52 +48:16:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125211_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 125211_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 131365_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 131365_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:43:48.20 +49:16:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76476_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 76476_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:49:29.38 +45:29:52.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 136881_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 136881_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 30673_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 30673_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:14:44.16 +42:22:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192623_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 192623_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:54:04.27 +44:33:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108129_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
Preparing report for the candidate 108129_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
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Considering the candidate 49422_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 49422_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:23:35.27 +43:39:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59284_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 59284_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:17:47.60 +44:01:31.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 85267_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 85267_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:16:04.86 +45:20:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45831_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 45831_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:21:26.71 +43:19:50.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141017_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 141017_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:13:24.12 +48:10:35.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 34044_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 34044_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
**** FOUND 03:14:56.85 +42:30:14.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165839_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001
The candidate 165839_fd_Per-02-Q2b1x1_2026-04-09_22-27-28_20.00sec_-5.00C_LIGHT_0001 did not pass the final checks
