This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041929.18+574348.0,2461136.7307,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J041929.18+574348.0 20260406.2307 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IX Cam,2461136.7307,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
IX Cam 20260406.2307 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045356.18+582712.9,2461136.7307,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J045356.18+582712.9 20260406.2307 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0419084+573821,2461136.7307,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0419084+573821 20260406.2307 10.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TZ Cam,2461136.7307,8.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
TZ Cam 20260406.2307 8.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7307,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2307 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7307,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2307 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7307,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2307 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050518.62+613049.7,2461136.7307,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J050518.62+613049.7 20260406.2307 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0440167+593502,2461136.7307,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0440167+593502 20260406.2307 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0438578+573332,2461136.7307,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0438578+573332 20260406.2307 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J042445.99+621242.9,2461136.7307,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J042445.99+621242.9 20260406.2307 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0400273+642548,2461136.7307,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0400273+642548 20260406.2307 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2175143,2461136.7307,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2175143 20260406.2307 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042715.10+570205.7,2461136.7307,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J042715.10+570205.7 20260406.2307 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0442423+640229,2461136.7307,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0442423+640229 20260406.2307 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 03745-01205,2461136.7307,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
GSC 03745-01205 20260406.2307 12.16CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2131605,2461136.7307,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2131605 20260406.2307 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J051033.92+591344.9,2461136.7307,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J051033.92+591344.9 20260406.2307 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 278767571062765056,2461136.7307,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 278767571062765056 20260406.2307 12.47CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0420475+623457,2461136.7307,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0420475+623457 20260406.2307 13.53CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0525045+600235,2461136.7307,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J0525045+600235 20260406.2307 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J041708.74+613657.9,2461136.7307,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J041708.74+613657.9 20260406.2307 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.7307,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.2307 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045206.63+583804.6,2461136.7307,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J045206.63+583804.6 20260406.2307 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 475419520661019776,2461136.7307,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 475419520661019776 20260406.2307 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J045050.81+645248.1,2461136.7307,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 J045050.81+645248.1 20260406.2307 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BH Cam,2461136.7307,8.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
BH Cam 20260406.2307 8.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 2110062,2461136.7307,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 2110062 20260406.2307 12.46CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461136.73111639 06.04.2026 05:32:38.456 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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): 18331
Objects passed selection criteria: 18281
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 14748.2
Average stars matched: 14186.8 (96.1928 %)
Memory usage VmPeak: 121968 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 00:58:58 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
First image: 2461049.69737530 09.01.2026 04:44:03.226 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Last image: 2461136.73111639 06.04.2026 05:32:38.456 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 65 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): 122643
Objects passed selection criteria: 122351
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 92555
Average stars matched: 88608.8 (95.7363 %)
Memory usage VmPeak: 2670872 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 01:01:44 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.73030639
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
Saving wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits to local_wcs_cache/
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
Saving wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits to local_wcs_cache/
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits'
wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits exists and is non-empty
Saving wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits to local_wcs_cache/
'wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits' -> 'local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:44.240 +61:59:01.74
Angular distance between the image centers 0.0343 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:41.636 +61:58:31.22
Angular distance between the image centers 0.0343 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:08:44.240 +61:59:01.74
Second-epoch second image center 05:08:41.636 +61:58:31.22
Angular distance between the image centers 0.00989 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/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.2YiHXiTybT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.RrLTNTxow4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits &> /tmp/tmp.18rqKl3NMx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits &> /tmp/tmp.6Ee6OOeKQa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
The reference image (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat) found
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 18409 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 57.0231 to 95.6672 deg, Dec +55.2649 to +67.4913 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 57.0231 to 95.6672 deg, Dec 55.2649 to 67.4913 deg
Loaded 14048 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): 8129 out of 8891 total matches.
Matched with Tycho-2 8891 out of 18409 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955063
a=0.000000 b=1.000000 c=22.955063
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
2.0 pix Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
4.1 pix fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
4.1 pix fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Limiting magnitude estimates:
15.5 mag. Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.5 mag. Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
14.4 mag. fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
14.4 mag. fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2YiHXiTybT (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1604, passed=18409
Got 18409 stars (including 16782 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 18409 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18199 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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.RrLTNTxow4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1596, passed=18487
Got 18487 stars (including 16865 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 18487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18224 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 18223 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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.18rqKl3NMx (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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=567, passed=11300
Got 11300 stars (including 10727 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat
util/solve_plate_with_UCAC5 got 11300 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 11079 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 11079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 11079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits -region wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.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.6Ee6OOeKQa (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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=580, passed=11171
Got 11171 stars (including 10588 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat
util/solve_plate_with_UCAC5 got 11171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 10940 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 10940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 10940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits -region wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
Saving fully-calibrated image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits'
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits'
Preparing the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10547.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: 2s
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Considering the candidate 21283_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 21283_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:40:17.14 +66:08:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 0.588 483143555486324992 070.07160299110 +66.13472833216 9.6439 8.3302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21429_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 21429_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:19:45.99 +64:26:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21578_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 21578_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:07:24.09 +57:49:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21682_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 21682_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:57:26.35 +57:03:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 0.245 265701554697336448 089.35991692220 +57.06525020984 11.5101 10.9786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21798_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 21798_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:54:44.00 +64:34:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.971 479055743054112384 073.68330608219 +64.58065838646 10.8149 9.4761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21808_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 21808_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:51:30.28 +63:46:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04339_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 04339_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 09621_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 09621_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 20051_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 20051_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:40:17.08 +59:35:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.267 279081653432517248 070.07080093114 +59.58456181107 10.1153 8.5800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 03601_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 03601_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 04175_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 04175_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 10547_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 10547_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 10918_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 10918_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:35:17.96 +62:16:22.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:53:56.14 +58:27:14.0
04:19:08.72 +57:38:26.0
04:19:29.48 +57:43:50.6
05:10:46.04 +62:14:02.5
05:53:45.07 +63:00:49.7
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat to cache
SExtractor catalog cache: saved Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Creating symlink local_wcs_cache/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits exists and is non-empty
wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits exists and is non-empty
wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits exists and is non-empty
wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:44.240 +61:59:01.74
Angular distance between the image centers 0.0343 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:28.126 +61:59:49.99
Second-epoch image center 05:08:41.636 +61:58:31.22
Angular distance between the image centers 0.0343 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:08:44.240 +61:59:01.74
Second-epoch second image center 05:08:41.636 +61:58:31.22
Angular distance between the image centers 0.00989 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/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits &> /tmp/tmp.Z8ZFDaT34R
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits &> /tmp/tmp.JNvY5fLo9E
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits &> /tmp/tmp.Lij8CQ3ZL3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits &> /tmp/tmp.N9KkI64qsu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
Found non-empty wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits and wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
The reference image (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits) and catalog (wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat) found
'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat' -> 'wcsmag.cat'
Read 131449 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 56.9471 to 95.6842 deg, Dec +55.1951 to +67.5012 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 56.9471 to 95.6842 deg, Dec 55.1951 to 67.5012 deg
Loaded 14165 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): 6817 out of 9000 total matches.
Matched with Tycho-2 9000 out of 131449 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.808691
a=0.000000 b=1.000000 c=22.808691
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 99 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
1.9 pix Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
3.7 pix fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
3.6 pix fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Limiting magnitude estimates:
15.6 mag. Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
15.6 mag. Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
14.5 mag. fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
14.5 mag. fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
All-image limiting magnitude estimate: 14.5 (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.Z8ZFDaT34R (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=12667, passed=131418
Got 131418 stars (including 118531 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat
util/solve_plate_with_UCAC5 got 131418 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130184 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 130182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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.JNvY5fLo9E (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits' -> 'wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS_IMAGE_NAME=wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS-calibrated image found: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Checking if the catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits alredy exist and is non-empty...
Catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat corresponding to the image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
WCS catalog name: wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=12449, passed=130527
Got 130527 stars (including 117847 good ones) from the SExtractor catalog wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat
util/solve_plate_with_UCAC5 got 130527 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 129178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits -region wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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.Lij8CQ3ZL3 (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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=3669, passed=55444
Got 55444 stars (including 51729 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat
util/solve_plate_with_UCAC5 got 55444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 54364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 54364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 54364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits -region wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.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.N9KkI64qsu (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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
WCS-calibrated image found: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Checking if the catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat corresponding to the image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
WCS catalog name: wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=3519, passed=55415
Got 55415 stars (including 51860 good ones) from the SExtractor catalog wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat
util/solve_plate_with_UCAC5 got 55415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 54350 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 727 to 788 (Dec 55.5 to 67.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 54350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 54350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits -region wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.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_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-03_20.00sec_-15.00C_LIGHT_0171.fits
Saving fully-calibrated image wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_Cam-09-Q1b1x1_2026-01-08_22-44-43_20.00sec_-15.00C_LIGHT_0172.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-31-28_20.00sec_-5.00C_LIGHTs_0100.fits
Saving fully-calibrated image wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.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_2026-04-06_CI_Cam-09-Q1b1x1_003330_TTUQ1b1x1_27588_PtNNQVgu/wcs_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101.fits
Preparing the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out05303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out152470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95187.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 22s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 10s
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Considering the candidate 152426_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152426_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:15:04.43 +63:17:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.631 1007853490923155584 093.76931980102 +63.28703651408 13.8393 13.1428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152432_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 152432_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152435_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152435_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:52:06.36 +66:41:59.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)
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Considering the candidate 152436_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152436_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:19:54.88 +65:55:02.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 152440_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152440_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:47:18.45 +62:36:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 5.483 478561684375825152 071.82844109645 +62.60276932269 13.6464 12.8141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152442_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152442_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:16:50.01 +59:41:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.305 471848891011133184 064.20878688938 +59.69604710045 13.1007 12.5438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152443_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 152443_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152446_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152446_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:07:17.50 +63:50:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.080 476658120508983552 061.82227990774 +63.83850498530 13.1308 12.4496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152447_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152447_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:02:03.66 +63:24:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.233 476627918299464448 060.51315314570 +63.41630452616 13.0945 12.5060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152451_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152451_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:45:27.81 +60:36:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.282 471397232246381056 071.36421722776 +60.61529888561 13.5589 12.5929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152452_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152452_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:00:33.92 +60:57:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.561 1005847535038721536 090.14212395055 +60.96117880009 13.8402 13.2064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152453_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152453_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:22:02.05 +56:51:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.773 276898298224055296 065.50733172170 +56.85334491571 13.3149 12.5527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 152454_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152454_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:28:28.50 +56:52:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.539 278209706353203072 067.12148746868 +56.87380670989 13.1849 12.6258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152460_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152460_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:11:12.43 +59:18:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.475 470497350702120704 062.80302805063 +59.31294935059 12.7284 12.2810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152463_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152463_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:24:28.38 +66:31:21.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152468_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152468_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:48:38.98 +63:43:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 0.643 286892618396272512 087.16276742501 +63.72828275695 12.4897 11.9605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152469_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152469_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:03:21.78 +59:35:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152470_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152470_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:28:48.43 +65:17:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 1.300 477087995196306560 067.20179650975 +65.28674995511 11.2908 9.8488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152919_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 152919_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:06:21.09 +58:57:54.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153762_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 153762_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:46:55.76 +58:48:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.642 269968175209552768 086.73243601759 +58.80785149220 12.4901 11.5279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153822_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 153822_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:41:13.98 +58:04:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.049 269560737431553408 085.30612706082 +58.08329518948 12.9741 12.3747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153904_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 153904_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:03:07.97 +66:49:08.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153932_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 153932_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:12:27.98 +62:27:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154024_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154024_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:13:17.16 +62:42:03.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154080_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154080_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:10:53.01 +62:17:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.124 1006257584156033664 092.72115273167 +62.29799353706 12.7177 12.0046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154086_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154086_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:06:23.65 +63:12:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154314_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154314_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:47:06.33 +58:58:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154472_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154472_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:45:23.80 +56:58:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.805 268817192694618496 086.34955901679 +56.97098997464 12.8830 12.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154488_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154488_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:17:16.59 +57:50:30.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154697_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154697_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:06:12.67 +61:09:37.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154702_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154702_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:11:22.67 +60:26:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.396 1005654398948411136 092.84649869590 +60.43497283600 13.4893 12.9796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154739_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154739_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:14:52.61 +63:07:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154740_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154740_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:29:12.17 +62:41:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154878_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154878_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:42:32.16 +61:17:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.341 283446027400870528 085.63332374988 +61.28545693641 13.0822 12.4225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154918_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154918_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:00:31.90 +56:54:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.626 997510419399946112 090.13146085451 +56.90740691896 13.3319 12.5814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154960_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154960_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:12:01.64 +62:13:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.635 1006245901844969984 093.00643167723 +62.22363598278 13.4167 12.6771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154979_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 154979_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:55:26.31 +62:03:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.023 477617788000385664 073.86116723547 +62.04989778264 13.1854 12.6316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155175_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155175_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:43:24.54 +61:02:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.518 283238391501527552 085.85040509721 +61.04538151697 13.7951 13.1864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155190_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155190_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:44:20.87 +60:48:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.932 471456017462669696 071.08709451229 +60.80699524108 12.8703 11.8358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155242_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155242_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:58:23.95 +57:53:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.002 268801352855113216 089.60135862592 +57.89756618017 13.6580 12.8956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155261_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155261_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:03:42.23 +60:27:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.542 1005792795678495872 090.92480347479 +60.45388796725 13.6209 13.0625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155278_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155278_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:48:38.80 +59:31:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155285_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155285_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:46:38.70 +64:48:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.549 482114275164397952 071.66384874620 +64.81686125158 13.4799 12.5897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155337_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 155337_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 155414_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155414_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:32:33.66 +64:01:24.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 155568_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155568_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:05:12.39 +64:37:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.859 479202699654073600 076.30197933634 +64.62368812301 11.9978 9.9496 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155707_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155707_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:05:09.42 +60:10:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155802_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155802_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:39:53.77 +57:09:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 155953_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155953_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:34:42.03 +57:49:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.135 269490098105947520 083.67442695265 +57.82270442582 13.6082 12.7042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155975_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 155975_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:22:25.89 +60:19:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.652 284474964124334208 080.60859765007 +60.33299012905 13.8426 13.2585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156059_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 156059_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:03:16.79 +61:12:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.223 1005936664199718016 090.81906268723 +61.20641417869 14.0305 13.4324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156326_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 156326_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:22:21.89 +65:57:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.078 489352050971194368 065.58970917263 +65.95898736608 12.9446 11.3719 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156384_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 156384_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:48:38.62 +58:18:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.720 278066872919684352 072.16003618210 +58.31465826966 12.8297 11.1776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156572_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 156572_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:25:36.55 +59:49:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.888 282884211317850624 081.40274824485 +59.82461786548 13.7825 12.9314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20143_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 20143_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:00:03.02 +58:26:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 147776_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 147776_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:50:36.35 +58:17:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62952_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 62952_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 44559_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 44559_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 19902_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 19902_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 100048_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 100048_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 95187_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 95187_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 124534_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 124534_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:31:43.76 +64:14:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114638_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 114638_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 18490_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 18490_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 118109_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 118109_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 35828_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 35828_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 17362_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 17362_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
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Considering the candidate 32261_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 32261_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121037_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 121037_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:19:45.99 +64:26:01.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123975_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 123975_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:51:30.32 +63:46:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92395_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 92395_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:19:52.04 +63:15:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29771_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 29771_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:19:08.74 +57:38:25.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28374_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 28374_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127816_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 127816_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40460_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 40460_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05303_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 05303_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 06:00:10.82 +57:18:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.485 997546630267842048 090.04473830106 +57.31382791738 13.7803 13.2322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81364_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 81364_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74969_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 74969_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73386_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 73386_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:23:29.00 +62:29:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29216_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 29216_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 81854_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 81854_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:35:17.99 +62:16:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92193_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 92193_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25949_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 25949_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:32:40.18 +58:57:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142047_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 142047_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:12:27.97 +63:01:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30992_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 30992_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:19:29.49 +57:43:50.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78569_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 78569_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:53:45.06 +63:00:49.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109716_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 109716_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 99023_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 99023_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:03:12.31 +64:13:11.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103232_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 103232_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:33:39.07 +62:33:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25460_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 25460_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:53:56.13 +58:27:13.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113950_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 113950_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71135_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 71135_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:10:46.06 +62:14:02.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23430_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
Preparing report for the candidate 23430_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28304_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 28304_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:27:46.23 +57:49:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46344_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 46344_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 05:03:25.05 +60:26:35.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126795_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 126795_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:52:05.78 +63:30:16.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89933_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 89933_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:54:03.22 +66:20:29.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95727_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 95727_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:20:40.71 +65:08:24.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65521_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101
The candidate 65521_fd_Cam-09-Q1b1x1_2026-04-06_00-32-38_20.00sec_-4.90C_LIGHTs_0101 did not pass the final checks
**** FOUND 04:21:48.28 +60:44:08.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 34s
Prepared the HTML report for the field Cam-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:53:56.14 +58:27:14.0
04:19:08.72 +57:38:26.0
04:19:29.48 +57:43:50.6
05:10:46.04 +62:14:02.5
05:53:45.07 +63:00:49.7
04:24:46.24 +62:12:43.4
04:50:50.86 +64:52:47.2
05:55:02.15 +64:58:40.8
04:54:44.01 +64:34:49.2
04:42:42.73 +64:02:29.3
04:20:47.22 +62:34:58.9
05:04:45.89 +59:35:48.0
04:08:40.67 +59:05:50.5
05:50:59.30 +65:46:39.5
04:52:02.18 +57:44:30.9
04:27:15.31 +57:02:08.2
04:38:58.15 +57:33:35.5
04:25:20.27 +57:20:32.4
04:40:58.48 +58:17:11.4
04:52:06.53 +58:38:05.1
05:10:33.77 +59:13:45.5
04:46:30.96 +59:02:44.7
05:25:04.32 +60:02:32.9
04:40:17.14 +59:35:05.7
05:05:18.65 +61:30:51.1
04:11:40.46 +60:50:38.0
04:17:09.03 +61:36:58.6
04:10:03.64 +61:30:24.3
04:00:27.68 +64:25:45.9
########### Completed Cam-09-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
04:19:29.48 +57:43:50.6
05:10:46.04 +62:14:02.5
04:53:56.14 +58:27:14.0
04:19:08.72 +57:38:26.0
05:53:45.07 +63:00:49.7
05:04:45.89 +59:35:48.0
04:08:40.67 +59:05:50.5
05:50:59.30 +65:46:39.5
05:05:18.65 +61:30:51.1
04:40:17.14 +59:35:05.7
04:38:58.15 +57:33:35.5
04:24:46.24 +62:12:43.4
04:00:27.68 +64:25:45.9
04:54:44.01 +64:34:49.2
04:27:15.31 +57:02:08.2
04:42:42.73 +64:02:29.3
04:46:30.96 +59:02:44.7
04:52:02.18 +57:44:30.9
05:10:33.77 +59:13:45.5
04:40:58.48 +58:17:11.4
04:20:47.22 +62:34:58.9
05:25:04.32 +60:02:32.9
04:17:09.03 +61:36:58.6
04:11:40.46 +60:50:38.0
04:52:06.53 +58:38:05.1
04:10:03.64 +61:30:24.3
04:50:50.86 +64:52:47.2
05:55:02.15 +64:58:40.8
04:25:20.27 +57:20:32.4
###################################################################################
04:19:29.48 +57:43:50.6 -- not an asteroid (will add it to exclusion list)
05:10:46.04 +62:14:02.5 -- not an asteroid (will add it to exclusion list)
04:53:56.14 +58:27:14.0 -- not an asteroid (will add it to exclusion list)
04:19:08.72 +57:38:26.0 -- not an asteroid (will add it to exclusion list)
05:53:45.07 +63:00:49.7 -- not an asteroid (will add it to exclusion list)
05:04:45.89 +59:35:48.0 -- not an asteroid (will add it to exclusion list)
04:08:40.67 +59:05:50.5 -- not an asteroid (will add it to exclusion list)
05:50:59.30 +65:46:39.5 -- not an asteroid (will add it to exclusion list)
05:05:18.65 +61:30:51.1 -- not an asteroid (will add it to exclusion list)
04:40:17.14 +59:35:05.7 -- not an asteroid (will add it to exclusion list)
04:38:58.15 +57:33:35.5 -- not an asteroid (will add it to exclusion list)
04:24:46.24 +62:12:43.4 -- not an asteroid (will add it to exclusion list)
04:00:27.68 +64:25:45.9 -- not an asteroid (will add it to exclusion list)
04:54:44.01 +64:34:49.2 -- not an asteroid (will add it to exclusion list)
04:27:15.31 +57:02:08.2 -- not an asteroid (will add it to exclusion list)
04:42:42.73 +64:02:29.3 -- not an asteroid (will add it to exclusion list)
04:46:30.96 +59:02:44.7 -- not an asteroid (will add it to exclusion list)
04:52:02.18 +57:44:30.9 -- not an asteroid (will add it to exclusion list)
05:10:33.77 +59:13:45.5 -- not an asteroid (will add it to exclusion list)
04:40:58.48 +58:17:11.4 -- not an asteroid (will add it to exclusion list)
04:20:47.22 +62:34:58.9 -- not an asteroid (will add it to exclusion list)
05:25:04.32 +60:02:32.9 -- not an asteroid (will add it to exclusion list)
04:17:09.03 +61:36:58.6 -- not an asteroid (will add it to exclusion list)
04:11:40.46 +60:50:38.0 -- not an asteroid (will add it to exclusion list)
04:52:06.53 +58:38:05.1 -- not an asteroid (will add it to exclusion list)
04:10:03.64 +61:30:24.3 -- not an asteroid (will add it to exclusion list)
04:50:50.86 +64:52:47.2 -- not an asteroid (will add it to exclusion list)
05:55:02.15 +64:58:40.8 -- not an asteroid (will add it to exclusion list)
04:25:20.27 +57:20:32.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
04:00:27.68 +64:25:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:40.67 +59:05:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:03.64 +61:30:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:40.46 +60:50:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:09.03 +61:36:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:08.72 +57:38:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:29.48 +57:43:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:47.22 +62:34:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:46.24 +62:12:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:20.27 +57:20:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:15.31 +57:02:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:58.15 +57:33:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:17.14 +59:35:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:58.48 +58:17:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:42.73 +64:02:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:30.96 +59:02:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:50.86 +64:52:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:02.18 +57:44:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:06.53 +58:38:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:56.14 +58:27:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:44.01 +64:34:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:45.89 +59:35:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:18.65 +61:30:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:33.77 +59:13:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:46.04 +62:14:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:04.32 +60:02:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:59.30 +65:46:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:45.07 +63:00:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:02.15 +64:58:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
04:00:27.68 +64:25:45.9 -- a known variable star
04:08:40.67 +59:05:50.5 -- not a known variable star
04:10:03.64 +61:30:24.3 -- not a known variable star
04:11:40.46 +60:50:38.0 -- not a known variable star
04:17:09.03 +61:36:58.6 -- a known variable star
04:19:08.72 +57:38:26.0 -- a known variable star
04:19:29.48 +57:43:50.6 -- a known variable star
04:20:47.22 +62:34:58.9 -- a known variable star
04:24:46.24 +62:12:43.4 -- a known variable star
04:25:20.27 +57:20:32.4 -- a known variable star
04:27:15.31 +57:02:08.2 -- a known variable star
04:38:58.15 +57:33:35.5 -- a known variable star
04:40:17.14 +59:35:05.7 -- a known variable star
04:40:58.48 +58:17:11.4 -- a known variable star
04:42:42.73 +64:02:29.3 -- a known variable star
04:46:30.96 +59:02:44.7 -- a known variable star
04:50:50.86 +64:52:47.2 -- a known variable star
04:52:02.18 +57:44:30.9 -- a known variable star
04:52:06.53 +58:38:05.1 -- a known variable star
04:53:56.14 +58:27:14.0 -- a known variable star
04:54:44.01 +64:34:49.2 -- a known variable star
05:04:45.89 +59:35:48.0 -- not a known variable star
05:05:18.65 +61:30:51.1 -- a known variable star
05:10:33.77 +59:13:45.5 -- a known variable star
05:10:46.04 +62:14:02.5 -- a known variable star
05:25:04.32 +60:02:32.9 -- a known variable star
05:50:59.30 +65:46:39.5 -- not a known variable star
05:53:45.07 +63:00:49.7 -- a known variable star
05:55:02.15 +64:58:40.8 -- a known variable star
Found 5 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
29 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
04:00:27.68 +64:25:45.9
04:08:40.67 +59:05:50.5
04:10:03.64 +61:30:24.3
04:11:40.46 +60:50:38.0
04:17:09.03 +61:36:58.6
04:19:08.72 +57:38:26.0
04:19:29.48 +57:43:50.6
04:20:47.22 +62:34:58.9
04:24:46.24 +62:12:43.4
04:25:20.27 +57:20:32.4
04:27:15.31 +57:02:08.2
04:38:58.15 +57:33:35.5
04:40:17.14 +59:35:05.7
04:40:58.48 +58:17:11.4
04:42:42.73 +64:02:29.3
04:46:30.96 +59:02:44.7
04:50:50.86 +64:52:47.2
04:52:02.18 +57:44:30.9
04:52:06.53 +58:38:05.1
04:53:56.14 +58:27:14.0
04:54:44.01 +64:34:49.2
05:04:45.89 +59:35:48.0
05:05:18.65 +61:30:51.1
05:10:33.77 +59:13:45.5
05:10:46.04 +62:14:02.5
05:25:04.32 +60:02:32.9
05:50:59.30 +65:46:39.5
05:53:45.07 +63:00:49.7
05:55:02.15 +64:58:40.8
04:40:17.08 +59:35:05.5
04:40:17.14 +66:08:04.5
05:57:26.35 +57:03:54.9
04:54:44.00 +64:34:49.4
06:00:10.82 +57:18:53.2
06:15:04.43 +63:17:11.1
04:52:06.36 +66:41:59.5
05:19:54.88 +65:55:02.2
04:47:18.45 +62:36:14.8
04:16:50.01 +59:41:44.7
04:07:17.50 +63:50:16.8
04:02:03.66 +63:24:54.7
04:45:27.81 +60:36:58.2
06:00:33.92 +60:57:42.4
04:22:02.05 +56:51:17.3
04:28:28.50 +56:52:27.0
04:11:12.43 +59:18:47.6
05:24:28.38 +66:31:21.5
05:48:38.98 +63:43:41.5
04:28:48.43 +65:17:11.0
05:46:55.76 +58:48:30.9
05:41:13.98 +58:04:59.6
06:10:53.01 +62:17:53.8
05:45:23.80 +56:58:15.8
06:11:22.67 +60:26:09.9
05:42:32.16 +61:17:08.3
06:00:31.90 +56:54:30.3
06:12:01.64 +62:13:23.6
04:55:26.31 +62:03:02.7
05:43:24.54 +61:02:44.8
04:44:20.87 +60:48:27.1
05:58:23.95 +57:53:51.4
06:03:42.23 +60:27:15.5
04:46:38.70 +64:48:58.5
04:32:33.66 +64:01:24.6
05:05:12.39 +64:37:23.5
05:34:42.03 +57:49:23.4
05:22:25.89 +60:19:59.8
06:03:16.79 +61:12:21.5
04:22:21.89 +65:57:30.2
04:48:38.62 +58:18:53.2
05:25:36.55 +59:49:28.3
06:00:03.02 +58:26:33.3
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461136.73030639 -observatory V36
23:20:34.27 -06:24:47.2 Mercury (0.3mag)
02:21:40.46 +13:52:00.1 Venus (-3.9mag)
23:50:00.78 -02:11:54.5 Mars (1.2mag)
07:08:42.98 +22:52:25.6 Jupiter (-2.2mag)
00:24:46.68 +00:21:19.7 Saturn (0.9mag)
03:45:43.77 +19:41:07.0 Uranus (5.8mag)
00:09:32.07 -00:23:38.4 Neptune (7.8mag)
20:33:14.30 -22:52:29.3 Pluto (14.5mag)
16:00:53.53 -26:17:10.3 Moon (-11.5mag)
-rw-r--r-- 1 apache apache 362 Apr 6 00:58 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461136.73030639:
07:08:45.94 +22:52:16.9 Io (5.7mag)
07:08:55.58 +22:51:59.0 Europa (5.8mag)
07:08:38.00 +22:52:42.5 Ganymede (5.3mag)
07:08:13.03 +22:53:17.5 Callisto (6.5mag)
07:12:25.86 +22:44:54.5 Himalia (15.3mag)
07:08:41.33 +22:52:31.0 Thebe (16.2mag)
07:12:23.60 +23:13:41.0 Elara (17.2mag)
07:06:55.96 +23:37:32.7 Pasiphae (17.3mag)
07:17:14.75 +22:49:21.9 Carme (18.4mag)
00:24:41.47 +00:21:20.7 Titan (8.8mag)
00:24:43.44 +00:21:33.7 Rhea (10.1mag)
00:24:47.17 +00:22:53.0 Iapetus (11.5mag)
00:24:48.58 +00:21:08.0 Hyperion (14.8mag)
00:26:30.88 +00:31:08.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 00:59 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.73030639:
14:47:26.37 -08:21:31.6 JWST
17:03:51.77 +44:46:44.8 Chandra
08:05:17.47 -40:10:55.6 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 00:58 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.73030639 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:08.90 -28:14:15.0 14.0mag P/2010 H2 (Vales)
05:00:06.61 -70:08:45.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:34.54 +31:22:34.3 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.73 +09:22:29.3 17.6mag C/2021 G2 (ATLAS)
23:07:21.86 +28:52:09.8 17.0mag C/2022 E2 (ATLAS)
04:18:02.15 +25:45:55.4 15.9mag C/2022 N2 (PANSTARRS)
09:01:52.16 +31:54:26.0 16.1mag C/2022 QE78 (ATLAS)
08:29:59.33 -01:13:41.7 17.3mag C/2022 R6 (PANSTARRS)
18:55:35.03 +17:41:53.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:30.08 -11:39:36.0 17.6mag P/2023 B1 (PANSTARRS)
09:12:48.80 -13:29:47.8 17.5mag C/2023 F3 (ATLAS)
21:43:31.32 +62:22:23.5 17.5mag C/2023 H5 (Lemmon)
19:26:23.28 -03:36:32.0 14.3mag C/2023 R1 (PANSTARRS)
21:42:38.33 +84:36:56.7 17.8mag C/2023 X2 (Lemmon)
06:14:32.22 +63:34:59.9 17.0mag C/2024 A1 (ATLAS)
04:51:09.49 +14:34:21.4 10.4mag C/2024 E1 (Wierzchos)
16:25:04.92 +04:47:02.9 17.4mag C/2024 G6 (ATLAS)
20:17:33.84 +12:41:36.6 14.7mag C/2024 J3 (ATLAS)
03:17:47.97 -23:55:00.0 16.4mag C/2024 T5 (ATLAS)
05:08:44.07 +47:49:27.1 17.7mag C/2025 J1 (Borisov)
14:18:56.93 +37:25:49.9 14.8mag C/2025 L1 (ATLAS)
03:10:25.48 -24:45:16.1 17.8mag C/2025 Q3 (ATLAS)
22:53:40.73 +19:50:14.1 10.1mag C/2025 R3 (PANSTARRS)
12:58:22.49 +02:23:41.0 17.5mag C/2025 Y1 (ATLAS)
01:31:44.02 +04:41:51.1 7.2mag C/2026 A1 (MAPS)
23:30:55.52 +35:15:08.7 14.3mag C/2026 B2 (Sun-Gao)
18:23:52.02 -10:12:59.6 12.4mag 10P/Tempel
15:12:51.43 +04:06:32.4 13.1mag 24P/Schaumasse
11:05:45.47 -01:51:44.6 15.7mag 29P/Schwassmann-Wachmann
17:56:47.06 -09:59:29.2 17.7mag 40P/Vaisala
10:38:52.48 -04:56:40.4 16.7mag 43P/Wolf-Harrington
01:33:36.73 +15:48:10.3 17.1mag 47P/Ashbrook-Jackson
06:53:23.82 +39:04:22.0 17.0mag 63P/Wild
23:16:21.62 -12:39:00.6 15.7mag 65P/Gunn
03:37:46.54 +17:45:08.5 15.8mag 76P/West-Kohoutek-Ikemura
00:44:09.84 +06:17:34.4 14.4mag 78P/Gehrels
22:32:40.34 -12:15:36.7 14.5mag 88P/Howell
01:43:16.63 +17:57:30.2 15.1mag 93P/Lovas
04:36:59.64 +31:43:50.3 16.3mag 123P/West-Hartley
08:17:58.04 +42:52:22.5 16.2mag 124P/Mrkos
02:18:16.58 +13:15:41.2 16.4mag 128P/Shoemaker-Holt
02:28:28.43 +13:15:31.6 17.5mag 131P/Mueller
00:36:04.56 +09:37:30.6 11.2mag 141P/Machholz
00:46:02.84 +01:12:51.6 11.3mag 141P-A/Machholz
23:36:35.64 -02:24:38.6 14.0mag 141P-D/Machholz
01:15:10.49 +02:52:46.8 17.9mag 141P-I/Machholz
00:35:14.70 -06:23:55.2 15.2mag 162P/SidingSpring
10:30:57.81 +31:30:14.7 17.8mag 164P/Christensen
06:18:30.03 +24:31:19.8 17.8mag 198P/ODAS
15:08:38.07 -01:11:26.7 17.4mag 210P/Christensen
21:09:02.44 -13:48:43.4 17.4mag 218P/LINEAR
17:12:37.53 -15:04:07.7 16.2mag 235P/LINEAR
05:13:44.41 +33:51:35.1 16.6mag 240P/NEAT
07:34:12.93 -06:16:56.4 17.6mag 242P/Spahr
15:45:55.67 +06:18:43.4 17.5mag 391P/Kowalski
07:30:55.72 +21:18:43.0 17.6mag 450P/LONEOS
05:21:58.22 +45:36:32.3 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 00:59 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 6 00:58 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 6 00:58 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
09:20:25.810 +14:33:34.07 AT 2026huc 2026-03-17.76 20.65
06:44:02.780 +20:39:27.33 AT 2026hub 2026-03-18.72 20.62
13:08:33.600 +42:15:08.61 AT 2026hua 2026-03-15.75 21.43
13:21:41.610 +41:21:55.04 AT 2026htz 2026-03-15.75 21.4
13:27:29.400 +41:34:41.49 AT 2026hty 2026-03-15.75 21.81
13:19:37.170 +40:18:57.09 AT 2026htx 2026-03-15.75 21.98
13:07:58.480 +39:03:22.98 AT 2026htw 2026-03-15.75 21.29
13:33:30.740 +36:54:32.49 AT 2026htv 2026-03-15.74 21.49
13:44:31.540 +33:39:03.50 AT 2026htu 2026-03-15.74 21.57
13:38:22.690 +35:01:42.56 AT 2026htt 2026-03-15.74 21.92
13:18:28.600 +33:54:18.43 AT 2026hts 2026-03-15.74 22.06
13:14:14.650 +33:08:34.17 AT 2026htr 2026-03-15.74 21.29
13:18:12.570 +29:05:16.56 AT 2026htq 2026-03-15.74 21.89
-rw-r--r-- 1 apache apache 30K Apr 6 00:58 tns_transients_list.txt
