This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.45CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193252.13+071538.9,2461150.9644,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193252.13+071538.9 20260420.4644 12.58CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.0116+07.0484,2461150.9644,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.0116+07.0484 20260420.4644 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.2085+07.1492,2461150.9644,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.2085+07.1492 20260420.4644 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193215.57+072026.6,2461150.9644,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193215.57+072026.6 20260420.4644 12.01CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.0074+07.0072,2461150.9644,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.0074+07.0072 20260420.4644 12.58CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.2335+07.3339,2461150.9644,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.2335+07.3339 20260420.4644 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
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.66CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.9902+07.1070,2461150.9644,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.9902+07.1070 20260420.4644 12.73CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.0762+07.0986,2461150.9644,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.0762+07.0986 20260420.4644 12.33CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.1279+07.3818,2461150.9644,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.1279+07.3818 20260420.4644 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4644 2461150.9644 12.08 19:32:07.40 +07:01:10.8
43.86374 -5.75423 galactic Aql Second-epoch detections are separated by 0.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4295052959162496128 | 19:32:08.37 +07:00:35.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.589+/-0.033 (K)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4295052959162496128,2461150.9644,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4295052959162496128 20260420.4644 12.08CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295134151231529472,2461150.9644,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4295134151231529472 20260420.4644 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 20.4644 2461150.9644 12.47 19:32:21.49 +07:06:29.5
43.96985 -5.76353 galactic Aql Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4295106594700271360 | 19:32:21.49 +07:06:29.5 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.847+/-0.033 (M)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4295106594700271360,2461150.9644,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 4295106594700271360 20260420.4644 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.1646+07.4644,2461150.9644,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J293.1646+07.4644 20260420.4644 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295100100727411456,2461150.9644,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4295100100727411456 20260420.4644 12.66CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295052134492926976,2461150.9644,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4295052134492926976 20260420.4644 12.56CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461150.9644,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260420.4644 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.9184+07.0164,2461150.9644,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.9184+07.0164 20260420.4644 12.44CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193242.25+071739.2,2461150.9644,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193242.25+071739.2 20260420.4644 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.7667+06.8929,2461150.9644,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.7667+06.8929 20260420.4644 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J193151.61+070826.0,2461150.9644,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J193151.61+070826.0 20260420.4644 12.57CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295138957257802752,2461150.9644,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4295138957257802752 20260420.4644 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4295136831291157376,2461150.9644,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4295136831291157376 20260420.4644 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461150.96468665 20.04.2026 11:08:58.927 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
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: 4 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): 13993
Objects passed selection criteria: 13910
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 8759
Average stars matched: 8474.25 (96.7491 %)
Memory usage VmPeak: 120452 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 07:20:09 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: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
First image: 2461098.99883375 27.02.2026 11:58:09.236 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Last image: 2461150.96468665 20.04.2026 11:08:58.927 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 47 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): 168380
Objects passed selection criteria: 167869
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 112893
Average stars matched: 107649 (95.3551 %)
Memory usage VmPeak: 2003676 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 07:25:18 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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: 2461150.96406809
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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
Saving wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits to local_wcs_cache/
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits'
wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits exists and is non-empty
Saving wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits to local_wcs_cache/
'wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 942.3'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:42:51.800 +06:00:06.78 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits (1st new image)
verification OK: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:43:11.890 +05:58:53.67 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:43:11.890 +05:58:53.67
Angular distance between the image centers 0.0857 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
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# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits (2nd new image)
verification OK: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:43:13.095 +05:58:24.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:43:13.095 +05:58:24.84
Angular distance between the image centers 0.0927 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 19:43:11.890 +05:58:53.67
Second-epoch second image center 19:43:13.095 +05:58:24.84
Angular distance between the image centers 0.00944 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.by4zZ7AFjw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.G5x3PwZ6DO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits &> /tmp/tmp.aH6639pk0I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits &> /tmp/tmp.ru9CniPzaZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
The reference image (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat) found
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat' -> 'wcsmag.cat'
Read 19279 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.6603 to 303.6488 deg, Dec +0.6156 to +11.3108 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 287.6603 to 303.6488 deg, Dec 0.6156 to 11.3108 deg
Loaded 16831 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): 11809 out of 12562 total matches.
Matched with Tycho-2 12562 out of 19279 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779826
a=0.000000 b=1.000000 c=22.779826
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
2.1 pix Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
2.5 pix fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
2.5 pix fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Limiting magnitude estimates:
14.7 mag. Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
14.7 mag. Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
12.8 mag. fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
12.6 mag. fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 10.3 (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.by4zZ7AFjw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1674, passed=19279
Got 19279 stars (including 17574 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 19279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 18437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 964 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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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.G5x3PwZ6DO (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1629, passed=19357
Got 19357 stars (including 17702 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 19357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 18571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 18570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 18571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 965 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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.aH6639pk0I (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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=197, passed=4537
Got 4537 stars (including 4334 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 4537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4403 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 4401 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.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.ru9CniPzaZ (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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=204, passed=3629
Got 3629 stars (including 3423 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 3629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 3457 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
Saving fully-calibrated image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits'
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits'
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat to cache
SExtractor catalog cache: saved Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits exists and is non-empty
wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits exists and is non-empty
wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits (1st reference image)
verification OK: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Image size: 942.3'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:42:51.800 +06:00:06.78 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits (1st new image)
verification OK: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:43:11.890 +05:58:53.67 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:43:11.890 +05:58:53.67
Angular distance between the image centers 0.0857 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits (2nd new image)
verification OK: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Image size: 937.4'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 19:43:13.095 +05:58:24.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:42:51.800 +06:00:06.78
Second-epoch image center 19:43:13.095 +05:58:24.84
Angular distance between the image centers 0.0927 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 19:43:11.890 +05:58:53.67
Second-epoch second image center 19:43:13.095 +05:58:24.84
Angular distance between the image centers 0.00944 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/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits &> /tmp/tmp.R12ZBi14jK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.T2xjNEj9BX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits &> /tmp/tmp.8RVYi0Ut1S
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits &> /tmp/tmp.zdHJtecD04
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
Found non-empty wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits and wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
The reference image (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits) and catalog (wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat) found
'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat' -> 'wcsmag.cat'
Read 215901 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 287.6445 to 303.6494 deg, Dec +0.6156 to +11.3131 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 287.6445 to 303.6494 deg, Dec 0.6156 to 11.3131 deg
Loaded 16852 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): 11183 out of 14938 total matches.
Matched with Tycho-2 14938 out of 215901 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.584750
a=0.000000 b=1.000000 c=22.584750
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
1.9 pix Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
2.0 pix fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
2.1 pix fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Limiting magnitude estimates:
14.9 mag. Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
14.9 mag. Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
13.3 mag. fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
13.2 mag. fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.7 (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.R12ZBi14jK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=26960, passed=215867
Got 215867 stars (including 188619 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 215867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 209518 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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 209514 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 209515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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.T2xjNEj9BX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=27226, passed=216980
Got 216980 stars (including 189460 good ones) from the SExtractor catalog wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 216980 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 953 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 210127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 210126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 210123 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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.8RVYi0Ut1S (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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=3427, passed=55758
Got 55758 stars (including 52268 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 55758 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 53776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 53776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 53776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.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.zdHJtecD04 (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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS-calibrated image found: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Checking if the catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat corresponding to the image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
WCS catalog name: wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2682, passed=45287
Got 45287 stars (including 42551 good ones) from the SExtractor catalog wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 45287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 43320 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 43319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 43319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits -region wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_Aql-02-Q2b1x1_2026-02-27_05-58-09_20.00sec_-15.00C_LIGHT_0049.fits
Saving fully-calibrated image wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_Aql-02-Q2b1x1_2026-02-27_05-59-01_20.00sec_-14.90C_LIGHT_0050.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-05_20.00sec_-4.90C_LIGHT_0082.fits
Saving fully-calibrated image wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.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_2026-04-20_CI_Aql-02-Q2b1x1_062454_TTUQ2b1x1_1075688_7qSatyCC/wcs_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083.fits
Preparing the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out246115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out106920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138948.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 45s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 14s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246093_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246093_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:59:39.84 +07:40:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246115_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246115_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:54:35.55 +04:24:24.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246120_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246120_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:48:56.14 +02:12:18.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246154_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246154_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:30:10.91 +07:04:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.482 4294743549726702592 292.54583155983 +07.07601304213 10.3208 8.8118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246162_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246162_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 20:00:52.26 +07:19:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246175_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246175_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:32:19.63 +07:28:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.75, MAG_FAINT_SEARCH_LIMIT=11.73)GAIADR2_OUTPUT=# 0.209 4295153152149012864 293.08173822868 +07.46735733958 10.7776 9.7982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246218_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246218_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 20:00:50.04 +09:21:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246293_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246293_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 20:00:36.34 +08:26:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246306_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246306_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 20:00:55.36 +06:26:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.526 4249003316221522176 300.23081063298 +06.44155794617 12.1275 11.2889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246315_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246315_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 20:00:50.33 +09:18:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.010 4299979144877932928 300.20970980690 +09.31371975035 11.8790 11.1314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246372_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246372_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:32:05.97 +07:29:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.322 4295156416343635968 293.02587548629 +07.49814857652 13.0826 12.1592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246381_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246381_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:55:54.27 +10:13:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.838 4300327316414609920 298.97636096805 +10.21754163720 11.8600 11.3285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246409_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246409_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:45:53.04 +04:14:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246434_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246434_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:59:18.05 +09:29:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246490_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246490_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 20:00:24.73 +05:27:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 246524_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 246524_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:52:13.51 +07:28:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130630_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 130630_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134410_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 134410_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129743_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 129743_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131826_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 131826_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136241_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 136241_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128770_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 128770_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135871_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 135871_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106920_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 106920_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131007_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 131007_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131073_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 131073_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131682_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 131682_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137203_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 137203_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70827_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
The candidate 70827_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083 did not pass the final checks
**** FOUND 19:51:29.67 +04:27:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128890_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 128890_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134820_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 134820_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130836_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 130836_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128583_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 128583_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138948_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 138948_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 128939_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 128939_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136940_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 136940_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127849_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 127849_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136941_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 136941_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129952_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 129952_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129068_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 129068_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134932_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 134932_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126324_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 126324_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131695_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 131695_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136337_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 136337_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135034_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
Preparing report for the candidate 135034_fd_Aql-02-Q2b1x1_2026-04-20_06-08-58_20.00sec_-4.90C_LIGHT_0083
make_report_in_HTML.sh Phase 2 (HTML assembly): 2s
make_report_in_HTML.sh TOTAL: 61s
Prepared the HTML report for the field Aql-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:33:12.57 +06:03:32.4
19:31:04.35 +06:53:34.6
19:32:03.74 +06:57:31.6
19:31:28.14 +06:59:28.9
19:32:01.82 +07:00:38.3
19:32:07.40 +07:01:10.8
19:31:51.80 +07:01:12.4
19:31:37.38 +07:01:29.8
19:32:03.83 +07:03:27.1
19:31:59.29 +07:04:08.0
19:32:22.41 +07:06:02.1
19:32:21.49 +07:06:29.5
19:31:59.57 +07:06:54.8
19:32:17.60 +07:06:03.9
19:32:38.08 +07:08:36.5
19:31:53.05 +07:08:37.5
19:32:51.79 +07:09:18.5
19:32:54.03 +07:15:47.4
19:32:42.50 +07:17:04.2
19:32:42.97 +07:17:22.7
19:32:33.87 +07:17:57.0
19:32:55.27 +07:19:44.6
19:32:15.61 +07:20:25.1
19:32:54.14 +07:21:18.0
19:32:42.88 +07:22:42.5
19:32:45.42 +07:22:43.1
19:32:28.16 +07:23:19.4
19:32:37.88 +07:28:07.3
########### Completed Aql-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
19:32:22.41 +07:06:02.1
19:32:54.03 +07:15:47.4
19:32:03.83 +07:03:27.1
19:32:51.79 +07:09:18.5
19:32:15.61 +07:20:25.1
19:32:01.82 +07:00:38.3
19:32:55.27 +07:19:44.6
19:33:12.57 +06:03:32.4
19:31:59.57 +07:06:54.8
19:32:17.60 +07:06:03.9
19:32:38.08 +07:08:36.5
19:32:28.16 +07:23:19.4
19:32:07.40 +07:01:10.8
19:32:42.50 +07:17:04.2
19:32:21.49 +07:06:29.5
19:31:28.14 +06:59:28.9
19:32:37.88 +07:28:07.3
19:31:51.80 +07:01:12.4
19:32:42.88 +07:22:42.5
19:32:03.74 +06:57:31.6
19:32:45.42 +07:22:43.1
19:31:59.29 +07:04:08.0
19:31:37.38 +07:01:29.8
19:32:42.97 +07:17:22.7
19:31:04.35 +06:53:34.6
19:31:53.05 +07:08:37.5
19:32:54.14 +07:21:18.0
19:32:33.87 +07:17:57.0
###################################################################################
19:32:22.41 +07:06:02.1 -- not an asteroid (will add it to exclusion list)
19:32:54.03 +07:15:47.4 -- not an asteroid (will add it to exclusion list)
19:32:03.83 +07:03:27.1 -- not an asteroid (will add it to exclusion list)
19:32:51.79 +07:09:18.5 -- not an asteroid (will add it to exclusion list)
19:32:15.61 +07:20:25.1 -- not an asteroid (will add it to exclusion list)
19:32:01.82 +07:00:38.3 -- not an asteroid (will add it to exclusion list)
19:32:55.27 +07:19:44.6 -- not an asteroid (will add it to exclusion list)
19:33:12.57 +06:03:32.4 -- not an asteroid (will add it to exclusion list)
19:31:59.57 +07:06:54.8 -- not an asteroid (will add it to exclusion list)
19:32:17.60 +07:06:03.9 -- not an asteroid (will add it to exclusion list)
19:32:38.08 +07:08:36.5 -- not an asteroid (will add it to exclusion list)
19:32:28.16 +07:23:19.4 -- not an asteroid (will add it to exclusion list)
19:32:07.40 +07:01:10.8 -- not an asteroid (will add it to exclusion list)
19:32:42.50 +07:17:04.2 -- not an asteroid (will add it to exclusion list)
19:32:21.49 +07:06:29.5 -- not an asteroid (will add it to exclusion list)
19:31:28.14 +06:59:28.9 -- not an asteroid (will add it to exclusion list)
19:32:37.88 +07:28:07.3 -- not an asteroid (will add it to exclusion list)
19:31:51.80 +07:01:12.4 -- not an asteroid (will add it to exclusion list)
19:32:42.88 +07:22:42.5 -- not an asteroid (will add it to exclusion list)
19:32:03.74 +06:57:31.6 -- not an asteroid (will add it to exclusion list)
19:32:45.42 +07:22:43.1 -- not an asteroid (will add it to exclusion list)
19:31:59.29 +07:04:08.0 -- not an asteroid (will add it to exclusion list)
19:31:37.38 +07:01:29.8 -- not an asteroid (will add it to exclusion list)
19:32:42.97 +07:17:22.7 -- not an asteroid (will add it to exclusion list)
19:31:04.35 +06:53:34.6 -- not an asteroid (will add it to exclusion list)
19:31:53.05 +07:08:37.5 -- not an asteroid (will add it to exclusion list)
19:32:54.14 +07:21:18.0 -- not an asteroid (will add it to exclusion list)
19:32:33.87 +07:17:57.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:31:04.35 +06:53:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:28.14 +06:59:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:37.38 +07:01:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:51.80 +07:01:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:53.05 +07:08:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:59.29 +07:04:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:59.57 +07:06:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:01.82 +07:00:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:03.74 +06:57:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:03.83 +07:03:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:07.40 +07:01:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:15.61 +07:20:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:17.60 +07:06:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:21.49 +07:06:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:22.41 +07:06:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:28.16 +07:23:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:33.87 +07:17:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:37.88 +07:28:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:38.08 +07:08:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:42.50 +07:17:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:42.88 +07:22:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:42.97 +07:17:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:45.42 +07:22:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:51.79 +07:09:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:54.03 +07:15:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:54.14 +07:21:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:55.27 +07:19:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:12.57 +06:03:32.4 -- 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)
19:31:04.35 +06:53:34.6 -- not a known variable star
19:31:28.14 +06:59:28.9 -- not a known variable star
19:31:37.38 +07:01:29.8 -- not a known variable star
19:31:51.80 +07:01:12.4 -- a known variable star
19:31:53.05 +07:08:37.5 -- a known variable star
19:31:59.29 +07:04:08.0 -- not a known variable star
19:31:59.57 +07:06:54.8 -- not a known variable star
19:32:01.82 +07:00:38.3 -- not a known variable star
19:32:03.74 +06:57:31.6 -- a known variable star
19:32:03.83 +07:03:27.1 -- not a known variable star
19:32:07.40 +07:01:10.8 -- not a known variable star
19:32:15.61 +07:20:25.1 -- a known variable star
19:32:17.60 +07:06:03.9 -- not a known variable star
19:32:21.49 +07:06:29.5 -- not a known variable star
19:32:22.41 +07:06:02.1 -- not a known variable star
19:32:28.16 +07:23:19.4 -- not a known variable star
19:32:33.87 +07:17:57.0 -- a known variable star
19:32:37.88 +07:28:07.3 -- not a known variable star
19:32:38.08 +07:08:36.5 -- not a known variable star
19:32:42.50 +07:17:04.2 -- a known variable star
19:32:42.88 +07:22:42.5 -- not a known variable star
19:32:42.97 +07:17:22.7 -- a known variable star
19:32:45.42 +07:22:43.1 -- not a known variable star
19:32:51.79 +07:09:18.5 -- not a known variable star
19:32:54.03 +07:15:47.4 -- not a known variable star
19:32:54.14 +07:21:18.0 -- a known variable star
19:32:55.27 +07:19:44.6 -- not a known variable star
19:33:12.57 +06:03:32.4 -- not a known variable star
Found 20 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
28 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 ####
19:31:04.35 +06:53:34.6
19:31:28.14 +06:59:28.9
19:31:37.38 +07:01:29.8
19:31:51.80 +07:01:12.4
19:31:53.05 +07:08:37.5
19:31:59.29 +07:04:08.0
19:31:59.57 +07:06:54.8
19:32:01.82 +07:00:38.3
19:32:03.74 +06:57:31.6
19:32:03.83 +07:03:27.1
19:32:07.40 +07:01:10.8
19:32:15.61 +07:20:25.1
19:32:17.60 +07:06:03.9
19:32:21.49 +07:06:29.5
19:32:22.41 +07:06:02.1
19:32:28.16 +07:23:19.4
19:32:33.87 +07:17:57.0
19:32:37.88 +07:28:07.3
19:32:38.08 +07:08:36.5
19:32:42.50 +07:17:04.2
19:32:42.88 +07:22:42.5
19:32:42.97 +07:17:22.7
19:32:45.42 +07:22:43.1
19:32:51.79 +07:09:18.5
19:32:54.03 +07:15:47.4
19:32:54.14 +07:21:18.0
19:32:55.27 +07:19:44.6
19:33:12.57 +06:03:32.4
19:54:35.55 +04:24:24.9
19:48:56.14 +02:12:18.1
19:30:10.91 +07:04:33.0
19:32:19.63 +07:28:02.4
20:00:55.36 +06:26:29.5
20:00:50.33 +09:18:49.4
19:32:05.97 +07:29:50.9
19:55:54.27 +10:13:03.1
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461150.96406809 -observatory V36
00:31:50.27 +00:35:27.8 Mercury (-0.1mag)
03:30:39.99 +19:27:04.1 Venus (-3.9mag)
00:30:30.73 +02:15:17.0 Mars (1.2mag)
07:14:45.84 +22:42:39.0 Jupiter (-2.1mag)
00:31:09.38 +01:01:14.4 Saturn (0.9mag)
03:48:39.26 +19:50:31.5 Uranus (5.8mag)
00:11:24.99 -00:11:45.2 Neptune (7.8mag)
20:33:55.83 -22:52:52.7 Pluto (14.5mag)
04:37:23.03 +26:20:11.7 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 362 Apr 20 07:20 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461150.96406809:
07:14:47.11 +22:42:33.7 Io (5.8mag)
07:14:58.14 +22:42:11.4 Europa (5.9mag)
07:14:39.72 +22:42:58.7 Ganymede (5.4mag)
07:14:45.19 +22:42:30.9 Callisto (6.6mag)
07:17:53.74 +22:28:17.0 Himalia (15.4mag)
07:14:47.00 +22:42:38.6 Thebe (16.3mag)
07:18:10.49 +22:58:37.1 Elara (17.3mag)
07:13:56.95 +23:20:19.2 Pasiphae (17.4mag)
07:22:59.37 +22:41:05.1 Carme (18.5mag)
00:31:00.09 +01:01:27.0 Titan (8.8mag)
00:31:06.99 +01:01:20.2 Rhea (10.1mag)
00:30:43.07 +01:00:41.0 Iapetus (11.5mag)
00:31:01.25 +01:01:39.6 Hyperion (14.8mag)
00:32:42.62 +01:09:33.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 20 07:20 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461150.96406809:
15:55:27.97 -19:14:45.6 JWST
18:33:07.77 +26:02:08.1 Chandra
09:17:51.17 -53:08:23.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 20 07:20 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461150.96406809 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:36.22 -29:02:57.8 13.9mag P/2010 H2 (Vales)
05:10:01.83 -69:27:23.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:28.02 +31:28:08.5 17.2mag C/2017 K2 (PANSTARRS)
17:29:53.37 +11:04:12.7 17.6mag C/2021 G2 (ATLAS)
23:11:20.32 +29:24:42.5 17.1mag C/2022 E2 (ATLAS)
04:34:28.90 +26:09:24.1 16.1mag C/2022 N2 (PANSTARRS)
09:04:30.75 +32:01:52.7 16.3mag C/2022 QE78 (ATLAS)
08:31:51.72 +00:18:28.6 17.4mag C/2022 R6 (PANSTARRS)
18:52:33.27 +18:54:05.5 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:09.09 -11:27:20.8 17.5mag P/2023 B1 (PANSTARRS)
09:05:43.90 -11:10:58.8 17.7mag C/2023 F3 (ATLAS)
21:58:27.95 +63:10:37.8 17.5mag C/2023 H5 (Lemmon)
19:14:59.91 -03:49:03.4 14.1mag C/2023 R1 (PANSTARRS)
21:19:51.85 +86:32:18.8 17.8mag C/2023 X2 (Lemmon)
06:20:15.43 +63:30:01.6 17.2mag C/2024 A1 (ATLAS)
05:22:37.19 +19:41:37.4 11.3mag C/2024 E1 (Wierzchos)
16:16:17.56 +07:07:03.9 17.3mag C/2024 G6 (ATLAS)
20:21:55.16 +16:30:16.8 14.5mag C/2024 J3 (ATLAS)
03:30:25.61 -21:43:05.7 16.3mag C/2024 T5 (ATLAS)
05:20:34.13 +44:12:30.4 17.7mag C/2025 J1 (Borisov)
13:20:32.27 +48:01:23.3 15.4mag C/2025 L1 (ATLAS)
03:32:29.46 -26:55:41.8 17.9mag C/2025 Q3 (ATLAS)
00:36:38.42 +15:59:38.9 8.0mag C/2025 R3 (PANSTARRS)
12:52:12.44 +03:16:31.7 17.4mag C/2025 Y1 (ATLAS)
03:59:54.22 +02:14:15.1 14.5mag C/2026 A1 (MAPS)
00:12:00.03 +38:00:08.8 14.7mag C/2026 B2 (Sun-Gao)
18:51:36.20 -09:28:36.1 11.6mag 10P/Tempel
14:54:11.83 +02:42:49.4 14.4mag 24P/Schaumasse
11:01:42.36 -01:23:21.3 15.7mag 29P/Schwassmann-Wachmann
10:37:36.91 -03:45:55.6 17.0mag 43P/Wolf-Harrington
01:55:36.14 +18:14:32.4 17.3mag 47P/Ashbrook-Jackson
07:19:09.54 +36:02:26.5 17.0mag 63P/Wild
23:34:41.09 -10:55:22.0 15.7mag 65P/Gunn
04:15:21.16 +22:44:50.3 15.9mag 76P/West-Kohoutek-Ikemura
01:15:30.12 +09:05:58.7 14.3mag 78P/Gehrels
23:16:19.68 -08:04:14.2 14.7mag 88P/Howell
02:23:10.85 +21:48:24.6 15.1mag 93P/Lovas
05:03:22.77 +32:30:49.5 16.1mag 123P/West-Hartley
08:33:52.05 +36:18:14.3 16.2mag 124P/Mrkos
02:40:09.58 +14:51:41.9 16.4mag 128P/Shoemaker-Holt
02:56:19.59 +15:01:29.2 17.5mag 131P/Mueller
01:49:53.65 +14:41:56.6 10.5mag 141P/Machholz
01:58:07.30 +06:32:03.6 10.5mag 141P-A/Machholz
00:41:28.11 +02:19:05.5 12.3mag 141P-D/Machholz
02:28:42.26 +08:17:01.0 17.9mag 141P-I/Machholz
01:14:52.95 +00:43:37.7 15.0mag 162P/SidingSpring
14:43:33.02 +00:21:19.2 17.8mag 210P/Christensen
21:51:22.24 -10:22:53.1 17.7mag 218P/LINEAR
17:17:17.45 -13:23:24.1 16.1mag 235P/LINEAR
05:44:12.88 +35:00:35.3 16.8mag 240P/NEAT
07:40:49.27 -04:42:01.2 17.8mag 242P/Spahr
22:28:04.91 -19:45:29.1 17.8mag 260P/McNaught
02:07:24.95 +21:34:36.1 18.0mag 295P/LINEAR
15:40:46.88 +07:16:20.8 17.5mag 391P/Kowalski
07:36:02.09 +21:22:23.3 17.7mag 450P/LONEOS
05:42:28.36 +44:46:17.7 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 20 07:20 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
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
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
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
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
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
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
-rw-r--r-- 1 apache apache 5.8K Apr 20 07:20 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 20 07:20 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:11:12.834 +13:54:28.45 AT 2026jkk 2026-04-11.95 20.07
11:55:00.280 +23:22:05.22 AT 2026jkj 2026-04-11.96 19.76
11:39:53.022 +10:43:26.76 AT 2026jki 2026-04-11.96 20.04
18:06:25.223 +11:52:09.71 AT 2026jkh 2026-04-12.15 19.52
16:50:00.163 +35:59:45.01 AT 2026jkg 2026-04-12.14 19.01
15:43:54.016 +44:51:51.60 SN 2026jkf 2026-04-12.14 18.53
11:24:19.761 -36:04:17.66 AT 2026jke 2026-04-06.51 19.98
11:16:25.694 -50:15:29.19 AT 2026jkd 2026-03-28.49 19.6
11:43:56.670 -49:03:17.42 AT 2026jkc 2026-04-12.46 19.35
11:38:21.891 -50:43:06.73 SN 2026jkb 2026-04-12.46 18.57
08:19:14.303 -28:43:36.53 AT 2026jka 2026-04-11.37 19.87
07:49:32.473 -24:44:26.65 AT 2026jjz 2026-04-12.39 18.98
14:44:18.498 -44:01:13.70 AT 2026jjy 2026-04-09.61 19.64
08:53:40.997 -38:26:31.85 AT 2026jjx 2026-03-23.40 20
12:26:02.763 -33:38:07.00 AT 2026jjw 2026-04-09.56 20.25
11:26:18.195 +19:38:31.94 AT 2026jjv 2026-04-06.91 19.81
11:33:29.132 -27:21:16.23 AT 2026jju 2026-04-12.45 19.32
12:15:03.964 -49:33:10.66 AT 2026jjt 2026-04-12.17 19.263
17:17:54.158 -75:07:32.46 AT 2026jjs 2026-04-12.30 19.194
08:35:23.434 +10:31:04.49 AT 2026jjr 2026-04-11.93 19.882
-rw-r--r-- 1 apache apache 30K Apr 20 07:20 tns_transients_list.txt
