This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.8779,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260402.3779 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DX Sco,2461132.8779,10.64,0.05,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
DX Sco 20260402.3779 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.8779,12.39,0.05,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
VARIABLE_NAME 20260402.3779 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.8779,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260402.3779 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FH Oph,2461132.8779,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FH Oph 20260402.3779 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ES Oph,2461132.8779,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ES Oph 20260402.3779 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0522 Oph,2461132.8779,11.31,0.05,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
V0522 Oph 20260402.3779 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174019.56-233028.6,2461132.8779,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174019.56-233028.6 20260402.3779 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BB Sco,2461132.8779,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BB Sco 20260402.3779 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 22670,2461132.8779,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 22670 20260402.3779 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173425.10-271005.2,2461132.8779,12.46,0.05,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
ASASSN-V J173425.10-271005.2 20260402.3779 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J172351-3008.5,2461132.8779,12.03,0.05,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
ASAS J172351-3008.5 20260402.3779 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CV Oph,2461132.8779,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CV Oph 20260402.3779 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173529.88-273307.6,2461132.8779,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173529.88-273307.6 20260402.3779 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173055-2719.1,2461132.8779,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173055-2719.1 20260402.3779 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J170613.00-301207.3,2461132.8779,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J170613.00-301207.3 20260402.3779 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J172200-2342.8,2461132.8779,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J172200-2342.8 20260402.3779 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173027-2645.4,2461132.8779,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173027-2645.4 20260402.3779 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4058734650191961088,2461132.8779,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4058734650191961088 20260402.3779 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AC Sco,2461132.8779,11.92,0.05,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
AC Sco 20260402.3779 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173917.47-223244.7,2461132.8779,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173917.47-223244.7 20260402.3779 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MU Oph,2461132.8779,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MU Oph 20260402.3779 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J171637-2820.8,2461132.8779,12.08,0.05,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
ASAS J171637-2820.8 20260402.3779 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174257.38-223607.1,2461132.8779,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174257.38-223607.1 20260402.3779 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IL Oph,2461132.8779,11.88,0.05,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
IL Oph 20260402.3779 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173648.70-283152.5,2461132.8779,12.57,0.05,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
ASASSN-V J173648.70-283152.5 20260402.3779 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173548-2854.7,2461132.8779,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173548-2854.7 20260402.3779 11.90CV 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: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461132.87813476 02.04.2026 09:04:20.843 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.37
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): 7743
Objects passed selection criteria: 7723
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 6433.75
Average stars matched: 6263.5 (97.3538 %)
Memory usage VmPeak: 114328 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:14:59 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: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
First image: 2461099.00968565 27.02.2026 12:13:46.840 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Last image: 2461132.87813476 02.04.2026 09:04:20.843 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 122
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: 24 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): 109985
Objects passed selection criteria: 109777
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 85139.5
Average stars matched: 81383.2 (95.5881 %)
Memory usage VmPeak: 1884056 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:17:55 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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: 2461132.87764146
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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits exists and is non-empty
Saving wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits to local_wcs_cache/
'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits'
wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits exists and is non-empty
Saving wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits to local_wcs_cache/
'wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:58.487 -26:00:30.82
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:58.840 -26:00:40.39
Angular distance between the image centers 0.04 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 17:16:58.487 -26:00:30.82
Second-epoch second image center 17:16:58.840 -26:00:40.39
Angular distance between the image centers 0.00297 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.ilNxdGAfFz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits &> /tmp/tmp.ougAThWUZk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.iaPkQEkghm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits &> /tmp/tmp.T6n7ucxAVL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
The reference image (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat) found
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat' -> 'wcsmag.cat'
Read 10772 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 250.0068 to 268.2094 deg, Dec -31.3083 to -20.4292 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 250.0068 to 268.2094 deg, Dec -31.3083 to -20.4292 deg
Loaded 11388 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): 7042 out of 7452 total matches.
Matched with Tycho-2 7452 out of 10772 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.815328
a=0.000000 b=1.000000 c=22.815328
From vast_summary.log: estimated ref. image limiting mag.: -8.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
2.1 pix Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
3.1 pix fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
3.1 pix fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Limiting magnitude estimates:
14.4 mag. Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
14.4 mag. Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
13.6 mag. fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
13.6 mag. fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ilNxdGAfFz (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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=949, passed=10772
Got 10772 stars (including 9801 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 10772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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.ougAThWUZk (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/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=936, passed=10621
Got 10621 stars (including 9668 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 10621 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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.iaPkQEkghm (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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=409, passed=5374
Got 5374 stars (including 4959 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 5374 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.T6n7ucxAVL (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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=394, passed=5422
Got 5422 stars (including 5025 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
util/solve_plate_with_UCAC5 got 5422 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.87"
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits -region wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
Saving fully-calibrated image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits'
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits'
Preparing the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out07146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20624.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20624_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 20624_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20660_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 20660_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:55:04.31 -25:52:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06085_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 06085_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:11:49.88 -26:39:11.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07146_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 07146_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Oph-08-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 ####
16:50:56.13 -25:10:39.0
16:48:32.84 -29:12:33.9
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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat to cache
SExtractor catalog cache: saved Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Creating symlink local_wcs_cache/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits exists and is non-empty
wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:58.487 -26:00:30.82
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:16:48.675 -26:00:08.00
Second-epoch image center 17:16:58.840 -26:00:40.39
Angular distance between the image centers 0.04 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 17:16:58.487 -26:00:30.82
Second-epoch second image center 17:16:58.840 -26:00:40.39
Angular distance between the image centers 0.00297 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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.UWKtAwSidf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits &> /tmp/tmp.f6byr4zDVG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.XWEQdnoqji
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits &> /tmp/tmp.WhF3yfLfXJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
Found non-empty wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits and wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
The reference image (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits) and catalog (wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat) found
'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat' -> 'wcsmag.cat'
Read 143168 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 249.9656 to 268.2487 deg, Dec -31.3138 to -20.3822 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 249.9656 to 268.2487 deg, Dec -31.3138 to -20.3822 deg
Loaded 11498 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): 8059 out of 9812 total matches.
Matched with Tycho-2 9812 out of 143168 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.596166
a=0.000000 b=1.000000 c=22.596166
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.57
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 88 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
1.8 pix Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
2.5 pix fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
2.6 pix fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Limiting magnitude estimates:
14.6 mag. Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
14.5 mag. Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
13.6 mag. fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
13.6 mag. fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UWKtAwSidf (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/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=11615, passed=143155
Got 143155 stars (including 131260 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 143155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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.f6byr4zDVG (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/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits' -> 'wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Checking if the catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat corresponding to the image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
WCS catalog name: wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=11364, passed=142792
Got 142792 stars (including 131150 good ones) from the SExtractor catalog wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 142792 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 937 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits -region wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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.XWEQdnoqji (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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3357, passed=52575
Got 52575 stars (including 49149 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 52575 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WhF3yfLfXJ (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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking if the catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS catalog name: wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3258, passed=51178
Got 51178 stars (including 47851 good ones) from the SExtractor catalog wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
util/solve_plate_with_UCAC5 got 51178 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits -region wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_Oph-08-Q2b1x1_2026-02-27_06-13-46_20.00sec_-15.00C_LIGHT_0067.fits
Saving fully-calibrated image wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_Oph-08-Q2b1x1_2026-02-27_06-14-28_20.00sec_-15.00C_LIGHT_0068.fits
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-03-38_20.00sec_-15.00C_LIGHT_0033.fits
Saving fully-calibrated image wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.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_2026-04-02_CI_Oph-08-Q2b1x1_041055_TTUQ2b1x1_32756_w96KKJPe/wcs_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034.fits
Preparing the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out116068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out120145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71149.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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: 13s
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Considering the candidate 167467_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167467_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:58:04.13 -28:01:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 5.056 6033169354158321920 254.51590148835 -28.01631021274 12.1644 10.2669 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167472_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167472_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:49:03.69 -25:03:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.286 6046804024204996736 252.26553350662 -25.06627151073 13.2158 12.7603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167480_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167480_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:47:59.15 -29:33:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 3.852 6031341690949073408 251.99524373423 -29.56541372531 12.4479 11.6713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167482_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167482_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:27:01.72 -28:41:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)
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Considering the candidate 167486_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167486_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:57:50.58 -22:12:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167488_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167488_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:36:17.53 -28:39:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 3.223 4060326017076602112 264.07213394941 -28.66292445336 11.1354 10.6103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167534_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167534_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:48:32.83 -29:12:34.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 167758_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167758_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:00:12.27 -24:58:00.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167775_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 167775_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
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Considering the candidate 167776_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167776_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:04:24.19 -23:22:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.398 4113705730389747968 256.09956872248 -23.37843430003 12.0533 11.1069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167780_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167780_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:05:34.89 -22:03:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.599 4115529403534574720 256.39507857289 -22.06551224575 12.2166 11.3020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167839_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167839_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:58:11.44 -23:31:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167850_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167850_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:08:46.65 -27:53:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167891_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167891_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:55:10.70 -21:56:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167911_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167911_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:55:11.77 -21:56:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.749 4126248542387842944 253.79895190053 -21.94319823820 12.3659 11.2300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167916_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167916_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:01:14.40 -25:42:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167926_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167926_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:04:02.02 -25:40:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167928_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167928_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:54:36.50 -29:05:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167931_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167931_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:00:29.39 -26:11:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167934_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167934_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:06:50.98 -26:29:42.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167935_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167935_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:15:09.76 -26:55:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167951_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167951_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:07:18.54 -28:11:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167954_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 167954_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
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Considering the candidate 167963_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167963_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:13:10.30 -30:03:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167973_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167973_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:08:02.98 -24:59:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.185 4112454554897439360 257.01261509471 -24.99886315892 12.5514 11.5004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167986_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167986_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:10:26.82 -29:10:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167990_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167990_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:29:50.99 -22:10:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 5.253 4117738494189396864 262.46088752020 -22.17050398972 11.5894 10.1403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167999_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 167999_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:40:14.12 -23:16:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168004_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168004_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:00:30.59 -26:45:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168013_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168013_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:09:25.32 -23:33:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.462 4112904456962049408 257.35505121924 -23.56421041394 13.3052 12.7732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168029_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168029_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:26:21.46 -29:50:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.049 4059435687543137536 261.58997764415 -29.84098944328 11.8476 10.2242 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168040_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168040_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:44:07.98 -27:18:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.191 4060789225042483456 266.03483818652 -27.31482448613 13.0577 10.9377 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 168042_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168042_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:37:21.69 -25:07:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168044_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168044_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:23:44.71 -24:49:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168057_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168057_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 168059_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168059_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:21:36.73 -26:21:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168060_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168060_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:18:11.27 -23:58:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168067_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 168067_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:00:17.61 -24:10:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.394 4113184699319163264 255.07265116460 -24.18072623428 13.8241 11.7411 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33974_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 33974_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:02:08.74 -28:59:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95049_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 95049_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:38:58.51 -25:03:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 3.730 4062174747138641664 264.74479701931 -25.05464480723 11.2916 9.6650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155223_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 155223_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:09:25.12 -28:26:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.942 4108415395891291392 257.35377179819 -28.43502567315 12.2498 10.4757 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 60742_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 60742_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:49:17.48 -27:12:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24051_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 24051_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:57:47.12 -29:29:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154393_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 154393_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:53:25.24 -22:10:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49148_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 49148_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
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Considering the candidate 45520_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 45520_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:09:00.25 -28:24:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116068_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 116068_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:41:25.38 -21:50:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.622 4117202138671612288 265.35622948828 -21.84779040336 11.9811 11.0412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 138228_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 138228_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:11:31.32 -24:28:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17781_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 17781_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
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Considering the candidate 139759_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 139759_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:01:49.19 -24:29:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121849_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 121849_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:32:01.77 -23:23:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71997_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 71997_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:11:49.90 -26:39:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29161_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 29161_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
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Considering the candidate 123786_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 123786_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
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Considering the candidate 92031_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 92031_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:07:10.95 -25:14:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16931_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 16931_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35283_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 35283_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112851_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 112851_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65439_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 65439_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16409_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 16409_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124624_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 124624_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:00:01.81 -23:25:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66623_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 66623_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60043_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 60043_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72426_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 72426_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:34:59.12 -26:40:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.464 4061776346014271488 263.74763073021 -26.67657895282 10.7759 9.1033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63227_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 63227_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14036_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 14036_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126555_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 126555_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80898_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 80898_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:55:04.32 -25:52:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71149_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 71149_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 158474_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 158474_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:10:49.39 -30:04:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40882_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 40882_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:03:38.47 -28:37:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21875_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 21875_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57059_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 57059_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 157666_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 157666_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:53:19.40 -24:58:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120145_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 120145_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:37:12.22 -22:07:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.702 4116850707274351872 264.30045037682 -22.12274739186 12.6417 11.9456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109480_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 109480_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66904_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 66904_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26023_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 26023_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:06:02.59 -29:28:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68045_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 68045_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:57:31.37 -26:48:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43863_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 43863_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:57:57.60 -28:23:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46888_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 46888_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110669_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 110669_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49621_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 49621_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127742_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 127742_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:55:48.69 -23:36:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73856_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 73856_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 17:18:19.10 -26:34:55.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39673_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
The candidate 39673_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034 did not pass the final checks
**** FOUND 16:52:35.12 -28:33:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44191_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 44191_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37405_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
Preparing report for the candidate 37405_fd_Oph-08-Q2b1x1_2026-04-02_04-04-20_20.00sec_-15.00C_LIGHT_0034
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 26s
Prepared the HTML report for the field Oph-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
16:50:56.13 -25:10:39.0
16:48:32.84 -29:12:33.9
17:39:17.37 -22:32:46.5
17:42:56.99 -22:36:12.6
17:40:19.20 -23:30:32.0
17:22:00.23 -23:42:47.9
17:06:13.12 -30:12:07.3
17:23:50.29 -30:08:10.4
16:56:55.39 -22:59:49.9
16:57:47.39 -23:15:13.3
16:46:03.28 -29:43:08.6
17:01:16.84 -29:54:50.2
17:31:40.67 -29:47:00.4
17:24:21.19 -29:24:07.5
17:34:34.52 -29:01:58.2
17:35:47.90 -28:54:43.5
17:36:48.54 -28:31:51.8
17:16:37.01 -28:20:50.3
17:02:32.28 -28:07:59.2
17:08:26.48 -28:09:35.4
16:46:35.76 -27:23:15.8
17:35:29.97 -27:33:06.5
17:30:54.21 -27:19:07.0
17:34:24.98 -27:10:05.0
16:55:46.05 -26:52:50.6
16:58:10.66 -26:53:35.9
17:30:26.82 -26:45:30.7
########### Completed Oph-08-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 ####
16:48:32.84 -29:12:33.9
16:50:56.13 -25:10:39.0
16:56:55.39 -22:59:49.9
16:57:47.39 -23:15:13.3
17:02:32.28 -28:07:59.2
17:01:16.84 -29:54:50.2
17:24:21.19 -29:24:07.5
17:40:19.20 -23:30:32.0
16:46:03.28 -29:43:08.6
17:34:34.52 -29:01:58.2
17:34:24.98 -27:10:05.0
17:23:50.29 -30:08:10.4
16:55:46.05 -26:52:50.6
17:35:29.97 -27:33:06.5
17:30:54.21 -27:19:07.0
17:06:13.12 -30:12:07.3
17:22:00.23 -23:42:47.9
17:30:26.82 -26:45:30.7
17:31:40.67 -29:47:00.4
16:46:35.76 -27:23:15.8
17:39:17.37 -22:32:46.5
16:58:10.66 -26:53:35.9
17:16:37.01 -28:20:50.3
17:42:56.99 -22:36:12.6
17:08:26.48 -28:09:35.4
17:36:48.54 -28:31:51.8
17:35:47.90 -28:54:43.5
###################################################################################
16:48:32.84 -29:12:33.9 -- asteroid (will NOT add it to exclusion list)
16:50:56.13 -25:10:39.0 -- not an asteroid (will add it to exclusion list)
16:56:55.39 -22:59:49.9 -- asteroid (will NOT add it to exclusion list)
16:57:47.39 -23:15:13.3 -- asteroid (will NOT add it to exclusion list)
17:02:32.28 -28:07:59.2 -- not an asteroid (will add it to exclusion list)
17:01:16.84 -29:54:50.2 -- not an asteroid (will add it to exclusion list)
17:24:21.19 -29:24:07.5 -- not an asteroid (will add it to exclusion list)
17:40:19.20 -23:30:32.0 -- not an asteroid (will add it to exclusion list)
16:46:03.28 -29:43:08.6 -- not an asteroid (will add it to exclusion list)
17:34:34.52 -29:01:58.2 -- not an asteroid (will add it to exclusion list)
17:34:24.98 -27:10:05.0 -- not an asteroid (will add it to exclusion list)
17:23:50.29 -30:08:10.4 -- not an asteroid (will add it to exclusion list)
16:55:46.05 -26:52:50.6 -- not an asteroid (will add it to exclusion list)
17:35:29.97 -27:33:06.5 -- not an asteroid (will add it to exclusion list)
17:30:54.21 -27:19:07.0 -- not an asteroid (will add it to exclusion list)
17:06:13.12 -30:12:07.3 -- not an asteroid (will add it to exclusion list)
17:22:00.23 -23:42:47.9 -- not an asteroid (will add it to exclusion list)
17:30:26.82 -26:45:30.7 -- not an asteroid (will add it to exclusion list)
17:31:40.67 -29:47:00.4 -- not an asteroid (will add it to exclusion list)
16:46:35.76 -27:23:15.8 -- not an asteroid (will add it to exclusion list)
17:39:17.37 -22:32:46.5 -- not an asteroid (will add it to exclusion list)
16:58:10.66 -26:53:35.9 -- not an asteroid (will add it to exclusion list)
17:16:37.01 -28:20:50.3 -- not an asteroid (will add it to exclusion list)
17:42:56.99 -22:36:12.6 -- not an asteroid (will add it to exclusion list)
17:08:26.48 -28:09:35.4 -- not an asteroid (will add it to exclusion list)
17:36:48.54 -28:31:51.8 -- not an asteroid (will add it to exclusion list)
17:35:47.90 -28:54:43.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
16:46:03.28 -29:43:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:46:35.76 -27:23:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
16:50:56.13 -25:10:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
16:55:46.05 -26:52:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
16:58:10.66 -26:53:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:01:16.84 -29:54:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:02:32.28 -28:07:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:06:13.12 -30:12:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:08:26.48 -28:09:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:37.01 -28:20:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:22:00.23 -23:42:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:23:50.29 -30:08:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:24:21.19 -29:24:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:30:26.82 -26:45:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:30:54.21 -27:19:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:31:40.67 -29:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:34:24.98 -27:10:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:34:34.52 -29:01:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:35:29.97 -27:33:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:35:47.90 -28:54:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:36:48.54 -28:31:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:39:17.37 -22:32:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:40:19.20 -23:30:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:42:56.99 -22:36:12.6 -- 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)
16:46:03.28 -29:43:08.6 -- a known variable star
16:46:35.76 -27:23:15.8 -- a known variable star
16:50:56.13 -25:10:39.0 -- a known variable star
16:55:46.05 -26:52:50.6 -- a known variable star
16:58:10.66 -26:53:35.9 -- a known variable star
17:01:16.84 -29:54:50.2 -- a known variable star
17:02:32.28 -28:07:59.2 -- a known variable star
17:06:13.12 -30:12:07.3 -- a known variable star
17:08:26.48 -28:09:35.4 -- a known variable star
17:16:37.01 -28:20:50.3 -- a known variable star
17:22:00.23 -23:42:47.9 -- a known variable star
17:23:50.29 -30:08:10.4 -- a known variable star
17:24:21.19 -29:24:07.5 -- a known variable star
17:30:26.82 -26:45:30.7 -- a known variable star
17:30:54.21 -27:19:07.0 -- a known variable star
17:31:40.67 -29:47:00.4 -- a known variable star
17:34:24.98 -27:10:05.0 -- a known variable star
17:34:34.52 -29:01:58.2 -- a known variable star
17:35:29.97 -27:33:06.5 -- a known variable star
17:35:47.90 -28:54:43.5 -- a known variable star
17:36:48.54 -28:31:51.8 -- a known variable star
17:39:17.37 -22:32:46.5 -- a known variable star
17:40:19.20 -23:30:32.0 -- a known variable star
17:42:56.99 -22:36:12.6 -- a known variable star
Found 0 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
24 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 ####
16:46:03.28 -29:43:08.6
16:46:35.76 -27:23:15.8
16:50:56.13 -25:10:39.0
16:55:46.05 -26:52:50.6
16:58:10.66 -26:53:35.9
17:01:16.84 -29:54:50.2
17:02:32.28 -28:07:59.2
17:06:13.12 -30:12:07.3
17:08:26.48 -28:09:35.4
17:16:37.01 -28:20:50.3
17:22:00.23 -23:42:47.9
17:23:50.29 -30:08:10.4
17:24:21.19 -29:24:07.5
17:30:26.82 -26:45:30.7
17:30:54.21 -27:19:07.0
17:31:40.67 -29:47:00.4
17:34:24.98 -27:10:05.0
17:34:34.52 -29:01:58.2
17:35:29.97 -27:33:06.5
17:35:47.90 -28:54:43.5
17:36:48.54 -28:31:51.8
17:39:17.37 -22:32:46.5
17:40:19.20 -23:30:32.0
17:42:56.99 -22:36:12.6
17:41:25.38 -21:50:52.3
17:37:12.22 -22:07:24.1
17:09:25.12 -28:26:05.3
16:58:04.13 -28:01:01.6
16:49:03.69 -25:03:57.4
16:47:59.15 -29:33:56.1
17:27:01.72 -28:41:42.7
17:36:17.53 -28:39:48.0
17:04:24.19 -23:22:44.1
17:05:34.89 -22:03:57.1
16:55:11.77 -21:56:36.2
17:08:02.98 -24:59:56.9
17:29:50.99 -22:10:13.4
17:09:25.32 -23:33:45.9
17:26:21.46 -29:50:26.5
17:44:07.98 -27:18:52.3
17:00:17.61 -24:10:50.9
17:34:59.12 -26:40:34.1
17:38:58.51 -25:03:18.5
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461132.87764146 -observatory V36
23:05:24.93 -07:28:46.6 Mercury (0.4mag)
02:03:34.30 +12:08:07.0 Venus (-3.9mag)
23:38:58.85 -03:24:22.0 Mars (1.2mag)
07:07:28.61 +22:54:16.1 Jupiter (-2.2mag)
00:23:01.27 +00:10:11.0 Saturn (0.9mag)
03:45:00.51 +19:38:45.2 Uranus (5.8mag)
00:09:00.44 -00:27:00.2 Neptune (7.8mag)
20:32:59.22 -22:52:38.1 Pluto (14.5mag)
12:50:57.08 -09:38:11.2 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 04:14 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461132.87764146:
07:07:36.64 +22:54:00.2 Io (5.7mag)
07:07:41.02 +22:53:52.0 Europa (5.8mag)
07:07:38.21 +22:53:50.3 Ganymede (5.3mag)
07:07:45.04 +22:53:35.3 Callisto (6.5mag)
07:11:18.35 +22:48:49.5 Himalia (15.3mag)
07:07:32.81 +22:54:08.0 Thebe (16.1mag)
07:11:10.39 +23:16:38.0 Elara (17.2mag)
07:05:25.94 +23:41:24.7 Pasiphae (17.3mag)
07:16:04.60 +22:50:42.2 Carme (18.4mag)
00:22:53.91 +00:10:36.0 Titan (8.8mag)
00:22:59.03 +00:10:18.5 Rhea (10.1mag)
00:23:10.54 +00:12:06.5 Iapetus (11.5mag)
00:22:51.66 +00:10:19.3 Hyperion (14.8mag)
00:24:48.09 +00:20:22.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 04:15 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.87764146:
14:22:21.41 -04:37:27.3 JWST
19:46:34.33 +06:10:01.8 Chandra
08:34:37.04 -47:29:52.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 04:15 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.87764146 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:45.30 -28:02:28.4 14.0mag P/2010 H2 (Vales)
04:57:44.35 -70:20:53.5 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.27 +31:21:18.3 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.76 +08:54:23.2 17.6mag C/2021 G2 (ATLAS)
23:06:05.71 +28:44:45.9 17.0mag C/2022 E2 (ATLAS)
04:13:44.44 +25:39:14.7 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.83 +31:49:51.4 16.1mag C/2022 QE78 (ATLAS)
08:29:48.57 -01:40:28.9 17.2mag C/2022 R6 (PANSTARRS)
18:56:02.48 +17:21:49.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:23.96 -11:42:37.3 17.6mag P/2023 B1 (PANSTARRS)
09:15:14.63 -14:09:25.9 17.5mag C/2023 F3 (ATLAS)
21:38:47.72 +62:11:16.7 17.4mag C/2023 H5 (Lemmon)
19:28:32.22 -03:34:41.3 14.3mag C/2023 R1 (PANSTARRS)
21:42:54.91 +84:08:55.3 17.8mag C/2023 X2 (Lemmon)
06:13:57.72 +63:37:28.0 17.0mag C/2024 A1 (ATLAS)
04:41:37.66 +12:46:02.6 10.1mag C/2024 E1 (Wierzchos)
16:27:04.49 +04:09:08.9 17.4mag C/2024 G6 (ATLAS)
20:16:00.13 +11:43:11.7 14.8mag C/2024 J3 (ATLAS)
03:14:33.17 -24:32:44.2 16.4mag C/2024 T5 (ATLAS)
05:05:48.39 +48:53:26.6 17.6mag C/2025 J1 (Borisov)
14:33:46.43 +33:17:19.7 14.7mag C/2025 L1 (ATLAS)
03:04:55.07 -24:12:53.9 17.7mag C/2025 Q3 (ATLAS)
22:45:37.61 +19:45:17.6 10.7mag C/2025 R3 (PANSTARRS)
13:00:02.09 +02:08:25.0 17.5mag C/2025 Y1 (ATLAS)
01:20:41.76 +02:40:51.4 8.4mag C/2026 A1 (MAPS)
23:19:04.27 +34:22:06.0 14.1mag C/2026 B2 (Sun-Gao)
18:16:19.48 -10:23:30.3 12.6mag 10P/Tempel
15:17:08.69 +04:23:54.2 12.8mag 24P/Schaumasse
11:07:06.57 -02:00:19.2 15.7mag 29P/Schwassmann-Wachmann
17:54:20.86 -10:08:58.8 17.6mag 40P/Vaisala
10:39:55.22 -05:18:47.3 16.6mag 43P/Wolf-Harrington
01:27:43.04 +15:07:38.6 17.1mag 47P/Ashbrook-Jackson
06:46:59.83 +39:51:49.0 17.1mag 63P/Wild
23:11:13.05 -13:08:13.6 15.7mag 65P/Gunn
03:28:06.72 +16:17:21.7 15.8mag 76P/West-Kohoutek-Ikemura
00:35:50.38 +05:31:23.0 14.5mag 78P/Gehrels
22:20:16.13 -13:22:04.4 14.5mag 88P/Howell
01:32:54.24 +16:51:32.8 15.1mag 93P/Lovas
04:30:21.31 +31:29:31.8 16.3mag 123P/West-Hartley
08:14:37.68 +44:38:52.2 16.2mag 124P/Mrkos
02:12:29.46 +12:48:51.9 16.4mag 128P/Shoemaker-Holt
02:21:01.69 +12:44:53.0 17.4mag 131P/Mueller
00:17:10.66 +08:05:52.7 11.6mag 141P/Machholz
00:27:21.16 -00:11:48.3 11.6mag 141P-A/Machholz
23:20:13.47 -03:35:10.7 14.5mag 141P-D/Machholz
00:55:48.00 +01:23:41.6 18.0mag 141P-I/Machholz
00:24:35.96 -08:17:06.7 15.3mag 162P/SidingSpring
10:32:24.09 +31:42:29.5 17.7mag 164P/Christensen
06:11:30.46 +24:36:03.5 17.8mag 198P/ODAS
15:15:06.69 -01:41:17.5 17.2mag 210P/Christensen
20:56:21.13 -14:44:08.4 17.3mag 218P/LINEAR
17:10:11.82 -15:29:14.0 16.2mag 235P/LINEAR
05:05:48.39 +33:28:10.4 16.5mag 240P/NEAT
07:32:51.53 -06:45:15.9 17.6mag 242P/Spahr
15:46:53.18 +06:01:45.1 17.6mag 391P/Kowalski
07:29:56.50 +21:16:34.3 17.6mag 450P/LONEOS
05:16:43.55 +45:50:25.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 04:15 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
-rw-r--r-- 1 apache apache 5.8K Apr 2 04:14 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
-rw-r--r-- 1 apache apache 187K Apr 2 04:14 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
08:53:19.672 -26:00:27.80 AT 2026hjm 2026-03-26.19 19.4129
-rw-r--r-- 1 apache apache 29K Apr 2 04:14 tns_transients_list.txt
