This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J083813-2252.0,2461139.5922,11.54,0.05,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 J083813-2252.0 20260409.0922 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5653804101306925568,2461139.5922,14.24,0.05,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 5653804101306925568 20260409.0922 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J130.2878-27.7201,2461139.5922,14.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J130.2878-27.7201 20260409.0922 14.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5645695138636722816,2461139.5922,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5645695138636722816 20260409.0922 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,14.03,0.05,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
target 20260409.0922 14.03CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5644927297266273920,2461139.5922,13.85,0.05,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 5644927297266273920 20260409.0922 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5693352370634439296,2461139.5922,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5693352370634439296 20260409.0922 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J132.2356-27.4732,2461139.5922,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J132.2356-27.4732 20260409.0922 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.57,0.05,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
target 20260409.0922 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J132.2143-27.5459,2461139.5922,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J132.2143-27.5459 20260409.0922 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J126.4712-24.5671,2461139.5922,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J126.4712-24.5671 20260409.0922 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J125.1628-28.6076,2461139.5922,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J125.1628-28.6076 20260409.0922 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5645213208948218112,2461139.5922,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5645213208948218112 20260409.0922 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.59,0.05,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
target 20260409.0922 13.59CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3689118,2461139.5922,13.41,0.05,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
DocumentRef: VOTx3689118 20260409.0922 13.41CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J085523.63-272018.8,2461139.5922,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J085523.63-272018.8 20260409.0922 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3720100,2461139.5922,13.24,0.05,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
DocumentRef: VOTx3720100 20260409.0922 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J131.8863-28.4542,2461139.5922,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J131.8863-28.4542 20260409.0922 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5655659290956667264,2461139.5922,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5655659290956667264 20260409.0922 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,12.92,0.05,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
target 20260409.0922 12.92CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J124.8634-25.2232,2461139.5922,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J124.8634-25.2232 20260409.0922 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J085728.51-240947.9,2461139.5922,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J085728.51-240947.9 20260409.0922 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5652380066248728192,2461139.5922,11.59,0.05,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 5652380066248728192 20260409.0922 11.59CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.48,0.05,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
target 20260409.0922 13.48CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5645273510286109312,2461139.5922,13.59,0.05,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 5645273510286109312 20260409.0922 13.59CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J125.6620-27.5867,2461139.5922,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J125.6620-27.5867 20260409.0922 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J082528.29-292932.5,2461139.5922,13.59,0.05,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
ASASSN-V J082528.29-292932.5 20260409.0922 13.59CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3778942,2461139.5922,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3778942 20260409.0922 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5646686004773473792,2461139.5922,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5646686004773473792 20260409.0922 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.5922,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.0922 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5648661861522954624,2461139.5922,14.11,0.05,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 5648661861522954624 20260409.0922 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5647033759684144128,2461139.5922,13.85,0.05,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 5647033759684144128 20260409.0922 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5642987866127864832,2461139.5922,14.02,0.05,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 5642987866127864832 20260409.0922 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J132.4507-22.7188,2461139.5922,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J132.4507-22.7188 20260409.0922 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J084558-2945.1,2461139.5922,12.02,0.05,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 J084558-2945.1 20260409.0922 12.02CV 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: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
First image: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Last image: 2461139.59249604 09.04.2026 02:13:01.658 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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.: -8.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 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): 16268
Objects passed selection criteria: 16188
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: 12000
Average stars matched: 10775.2 (89.7938 %)
Memory usage VmPeak: 120040 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 21:35:45 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: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
First image: 2461061.81789120 21.01.2026 07:37:35.800 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Last image: 2461139.59249604 09.04.2026 02:13:01.658 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 239
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
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: 73 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): 128246
Objects passed selection criteria: 127953
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 103041
Average stars matched: 91754.2 (89.0464 %)
Memory usage VmPeak: 1945020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 21:38:40 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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat to cache
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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: 2461139.59186795
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits exists and is non-empty
Saving wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits to local_wcs_cache/
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> 'local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits'
wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:38.038 -25:57:58.06
Angular distance between the image centers 0.0633 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 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:40.763 -25:58:01.88
Angular distance between the image centers 0.0714 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 08:38:38.038 -25:57:58.06
Second-epoch second image center 08:38:40.763 -25:58:01.88
Angular distance between the image centers 0.01026 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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits &> /tmp/tmp.2N8237aoQs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits &> /tmp/tmp.ptR0N0YwPC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits &> /tmp/tmp.IUqKkgosUZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits &> /tmp/tmp.8zpvrgsK27
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
The reference image (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits) and catalog (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat) found
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat' -> 'wcsmag.cat'
Read 20994 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6669 to 138.8549 deg, Dec -31.3522 to -20.3052 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 120.6669 to 138.8549 deg, Dec -31.3522 to -20.3052 deg
Loaded 21131 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): 13845 out of 14623 total matches.
Matched with Tycho-2 14623 out of 20994 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.840297
a=0.000000 b=1.000000 c=22.840297
From vast_summary.log: estimated ref. image limiting mag.: -8.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
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:
2.5 pix Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
2.4 pix Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
2.6 pix fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
2.6 pix fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Limiting magnitude estimates:
14.6 mag. Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
14.6 mag. Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
14.1 mag. fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
14.1 mag. fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2N8237aoQs (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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1631, passed=20994
Got 20994 stars (including 19342 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
util/solve_plate_with_UCAC5 got 20994 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 -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 20204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 936 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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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.ptR0N0YwPC (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/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1680, passed=20656
Got 20656 stars (including 18951 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
util/solve_plate_with_UCAC5 got 20656 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 -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 19523 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 19518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 19518 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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.IUqKkgosUZ (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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=942, passed=12235
Got 12235 stars (including 11281 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 12235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 11907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 11908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 11910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 931 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.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.8zpvrgsK27 (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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=965, passed=12489
Got 12489 stars (including 11511 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 12489 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 12062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 12063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 12064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
Saving fully-calibrated image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits'
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits'
Preparing the HTML report for the field Pyx-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out34414.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31063_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 31063_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:39:45.94 -29:33:17.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32664_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 32664_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:42.86 -25:14:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34414_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 34414_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05977_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 05977_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:24:25.98 -24:21:24.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 14s
Prepared the HTML report for the field Pyx-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:38:12.83 -22:51:58.4
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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat to cache
SExtractor catalog cache: saved Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Creating symlink local_wcs_cache/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Creating symlink local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
Creating symlink local_wcs_cache/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits exists and is non-empty
wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits exists and is non-empty
wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits exists and is non-empty
wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:38.038 -25:57:58.06
Angular distance between the image centers 0.0633 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 08:38:24.218 -26:00:09.42
Second-epoch image center 08:38:40.763 -25:58:01.88
Angular distance between the image centers 0.0714 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 08:38:38.038 -25:57:58.06
Second-epoch second image center 08:38:40.763 -25:58:01.88
Angular distance between the image centers 0.01026 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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits &> /tmp/tmp.KGyZjGc6Sn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits &> /tmp/tmp.VmstUmuruD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits &> /tmp/tmp.rjG8z6ngp6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits &> /tmp/tmp.C1cEZWfvZ6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
Found non-empty wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits and wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
The reference image (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits) and catalog (wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat) found
'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat' -> 'wcsmag.cat'
Read 149517 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 120.6583 to 138.9412 deg, Dec -31.3581 to -20.2738 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 120.6583 to 138.9412 deg, Dec -31.3581 to -20.2738 deg
Loaded 21265 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): 13597 out of 17470 total matches.
Matched with Tycho-2 17470 out of 149517 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.675683
a=0.000000 b=1.000000 c=22.675683
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.75
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 189 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
2.3 pix Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
2.2 pix fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
2.2 pix fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Limiting magnitude estimates:
14.7 mag. Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
14.8 mag. Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
14.2 mag. fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
14.3 mag. fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.KGyZjGc6Sn (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/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=17301, passed=149496
Got 149496 stars (including 131962 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat
util/solve_plate_with_UCAC5 got 149496 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 -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 145847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 145847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 145849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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.VmstUmuruD (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/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits' -> 'wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS-calibrated image found: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Checking if the catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat corresponding to the image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
WCS catalog name: wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=18384, passed=157885
Got 157885 stars (including 139292 good ones) from the SExtractor catalog wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat
util/solve_plate_with_UCAC5 got 157885 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 -31.4 to -20.3)
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...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 151938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 151939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 151937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits -region wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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.rjG8z6ngp6 (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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=9687, passed=108922
Got 108922 stars (including 99098 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 108922 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 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...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 105819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 105820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 105820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.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.C1cEZWfvZ6 (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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=10546, passed=111631
Got 111631 stars (including 100933 good ones) from the SExtractor catalog wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 111631 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 108382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 108382 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 108385 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits -region wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_Pyx-01-Q2b1x1_2026-01-21_01-37-35_20.00sec_-15.00C_LIGHT_0355.fits
Saving fully-calibrated image wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_Pyx-01-Q2b1x1_2026-01-21_01-38-48_20.00sec_-14.90C_LIGHT_0356.fits
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-12-07_20.00sec_-4.90C_LIGHT_0012.fits
Saving fully-calibrated image wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.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_2026-04-08_CI_Pyx-01-Q2b1x1_212429_TTUQ2b1x1_13972_N2hQXNPC/wcs_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013.fits
Preparing the HTML report for the field Pyx-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out173035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out173240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out173005.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out173041.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out173145.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out195308.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out196243.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out196918.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out198978.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out199154.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out199512.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out199706.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out199825.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out199884.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out200289.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out100249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199694.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 825s
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: 47s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172993_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 172993_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173001_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173001_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173003_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173003_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173005_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173005_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:23:55.78 -27:57:55.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173006_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173006_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:27:11.39 -25:31:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173009_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173009_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173018_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173018_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:40.83 -23:12:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173025_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173025_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173029_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173029_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173030_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173030_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173031_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173031_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173035_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173035_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:23.46 -28:59:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.297 5645379888038320512 129.59703251327 -28.98391313762 13.9055 13.1996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173041_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173041_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:20:46.45 -24:33:04.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173054_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173054_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173055_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173055_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173058_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173058_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173059_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173059_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:51:41.15 -23:48:18.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173061_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173061_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173079_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173079_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173080_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173080_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:32:44.22 -29:15:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173081_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173081_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:58:29.37 -27:29:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173086_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173086_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:30:46.84 -29:17:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173087_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173087_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173088_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173088_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:30.13 -29:53:26.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173092_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173092_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173094_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173094_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:16.18 -21:48:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173096_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173096_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173097_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173097_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:44:15.37 -25:42:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173102_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173102_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173107_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173107_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173111_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173111_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:49:49.16 -27:00:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173122_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173122_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173123_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173123_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:20:27.21 -29:17:36.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173125_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173125_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173127_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173127_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:21:39.55 -28:26:26.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173129_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173129_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:11.73 -27:19:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173130_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173130_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:27:06.77 -29:55:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173131_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173131_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:34:42.66 -29:11:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173139_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173139_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173142_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173142_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:23:55.13 -29:35:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173143_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173143_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:26.24 -29:03:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173145_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173145_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:49:56.80 -27:43:23.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173146_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173146_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173155_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173155_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173158_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173158_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173159_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173159_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:20:17.30 -26:43:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173162_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173162_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:40.29 -22:16:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173164_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173164_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:34:01.60 -28:20:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173167_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173167_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:45:03.72 -29:10:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173168_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173168_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173172_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173172_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173173_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173173_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173175_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173175_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:11.60 -29:07:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173179_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173179_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:21:17.93 -30:08:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173182_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173182_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173186_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173186_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:14.70 -25:59:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173187_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173187_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:27.46 -27:24:45.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173188_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173188_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173190_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173190_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:44:56.65 -25:46:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173194_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173194_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:42:58.07 -26:59:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173195_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173195_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:21:15.76 -24:20:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173196_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173196_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:45.34 -22:05:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173197_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173197_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:46:14.75 -22:52:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173198_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173198_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:45.32 -26:45:07.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173200_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173200_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:26:56.99 -29:30:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173202_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173202_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:54:17.46 -25:22:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.161 5652614704603998720 133.57242946179 -25.37249730208 12.9833 12.4530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173206_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173206_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:27:50.91 -30:08:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.672 5643928945008407808 126.96181588603 -30.14093536110 12.7985 12.3620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173209_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173209_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:45:06.33 -27:55:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173211_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173211_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:23:25.47 -29:29:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.983 5644411080859537792 125.85643317939 -29.49676893907 13.1108 12.9453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173212_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173212_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:31.10 -29:47:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173213_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173213_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:29:25.10 -30:10:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173216_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173216_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:23:55.59 -29:55:41.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173219_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173219_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:18:53.89 -27:25:42.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173221_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173221_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:48.97 -29:15:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173222_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173222_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:18:48.10 -29:46:16.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173223_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173223_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:26:59.73 -29:04:28.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173224_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173224_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:55:40.94 -29:10:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.802 5641807295576171520 133.92032820544 -29.17021537931 12.4228 11.9747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173228_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173228_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173235_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173235_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:53:20.84 -29:42:37.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173236_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173236_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:50:15.37 -28:52:50.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173238_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173238_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:02.81 -30:15:36.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173239_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173239_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:31.19 -21:53:48.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173240_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173240_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:11.03 -29:02:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 0.225 5644663517547082240 124.79597170822 -29.03450593525 11.5684 10.8552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173241_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 173241_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173242_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173242_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:23.36 -29:24:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173243_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 173243_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:43.95 -30:15:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178476_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 178476_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:39:01.98 -29:44:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178715_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 178715_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:44:30.31 -30:06:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179779_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 179779_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:45:55.45 -27:09:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180055_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 180055_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:33:05.19 -28:32:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180080_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 180080_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:51:36.50 -28:49:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180113_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 180113_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:40:55.98 -27:58:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180193_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 180193_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:44:45.55 -28:48:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180427_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 180427_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:20:10.29 -29:47:41.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181241_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 181241_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:44:35.06 -26:30:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181945_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 181945_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:36.23 -29:42:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182430_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 182430_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:42:45.11 -28:05:58.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182572_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 182572_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:03.13 -29:33:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182662_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 182662_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:01.83 -26:23:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 182669_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 182669_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:50:18.86 -28:52:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183019_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 183019_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:27.79 -26:56:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183369_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 183369_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:45:47.59 -25:41:41.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183866_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 183866_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:53:50.70 -29:33:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185128_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 185128_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:27:32.78 -28:07:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185147_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 185147_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:39:38.36 -26:29:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186003_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 186003_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:54:04.49 -27:52:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 186011_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 186011_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:28.42 -30:01:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187092_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 187092_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:53:19.13 -29:42:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 187884_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 187884_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:40.92 -29:56:23.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188052_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188052_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:35:36.34 -26:50:41.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188163_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188163_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:26:52.73 -29:14:02.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188341_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188341_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:31:32.36 -29:02:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.655 5644120878506107520 127.88502672896 -29.03501701873 13.3809 12.9435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188417_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188417_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:19.67 -28:41:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188563_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188563_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:28:37.44 -29:33:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188770_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188770_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:34:04.53 -25:53:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188970_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 188970_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:14.16 -30:04:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189463_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 189463_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:56:28.09 -25:28:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189472_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 189472_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:39:20.46 -29:27:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189770_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 189770_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:57.96 -26:27:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190442_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 190442_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:33:30.64 -26:58:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190654_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 190654_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:55:30.58 -27:19:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191101_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 191101_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:21:53.54 -22:58:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191180_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 191180_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:27:01.68 -29:35:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191212_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 191212_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:59.74 -28:14:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.891 5645700911072741376 129.49874841218 -28.23580191659 13.7134 13.0754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191364_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 191364_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:48:24.68 -27:07:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191485_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 191485_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:47:36.55 -25:59:31.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191657_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 191657_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:28.91 -28:47:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192039_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 192039_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:26.17 -26:47:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192499_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 192499_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:19.48 -28:06:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192510_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 192510_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:57.82 -27:00:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192631_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 192631_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:27.38 -28:06:45.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193439_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 193439_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:40:14.33 -24:19:29.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193862_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 193862_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194332_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 194332_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194354_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 194354_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:39:47.41 -28:37:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194542_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 194542_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195030_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195030_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:46.11 -26:46:58.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195308_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195308_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:47:21.71 -28:48:43.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195432_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195432_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:09.20 -29:50:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195470_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195470_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:40:20.23 -26:59:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195561_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195561_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:04.21 -27:33:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195766_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195766_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:05.06 -28:50:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.910 5645420054570409472 130.27080007756 -28.84882677758 13.6340 13.1487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195939_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 195939_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:44:36.46 -26:00:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.644 5652377764146371840 131.15113076734 -25.99988236633 14.1738 13.7371 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196243_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 196243_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:43:56.66 -28:45:26.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196918_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 196918_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:32:52.71 -28:51:58.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197289_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 197289_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197380_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 197380_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197676_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 197676_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197781_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 197781_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:18:35.93 -26:38:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.627 5693624946440833792 124.64929854705 -26.63356840282 13.6486 13.1252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197793_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 197793_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197846_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 197846_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:51:37.92 -26:14:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.842 5652184795557824896 132.90681141611 -26.24815948409 14.2117 13.4276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197923_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 197923_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:45:20.76 -29:51:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198305_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 198305_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198384_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198384_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:31:47.30 -28:33:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.445 5646389269770967680 127.94653993659 -28.55040586340 13.7854 13.1279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198403_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198403_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:24:10.42 -28:40:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.085 5645035294222415744 126.04310941850 -28.66838505237 13.6485 12.8489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198471_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198471_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:49:04.13 -25:34:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 3.646 5652454695599622272 132.26690403718 -25.58219697609 14.4978 13.9870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198609_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198609_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:51:44.16 -28:25:04.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198636_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198636_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:34:47.16 -28:35:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.582 5645649302749350144 128.69625674628 -28.59094918269 13.0666 10.7870 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198638_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198638_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:13.13 -29:55:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198747_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198747_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:57.76 -28:05:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 2.762 5648716905823269760 133.24033291638 -28.08659705485 13.9181 13.2156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198970_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198970_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:49:18.84 -28:23:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198978_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 198978_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:50:04.75 -30:02:11.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199083_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199083_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:51:45.58 -29:04:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.508 5642595306117544320 132.93947965545 -29.08157813612 14.0117 13.4303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199154_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199154_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:47:42.53 -29:34:51.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199162_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199162_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:02.13 -27:59:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.268 5645915105379295872 130.25847604694 -27.99041963992 13.8488 13.1303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199255_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 199255_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199490_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 199490_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199512_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199512_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:56:28.64 -26:33:52.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199519_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199519_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:47.86 -29:37:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199694_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 199694_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199706_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199706_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:32:27.06 -30:10:19.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199825_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199825_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:19.88 -28:21:33.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199862_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199862_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:33.89 -29:22:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.831 5641833928675724544 133.14030885952 -29.37200798948 14.1125 13.6013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199884_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 199884_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:30:47.64 -29:30:01.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200077_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 200077_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:07.91 -26:37:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 3.494 5646338627812677632 130.28205245796 -26.62807619509 14.3241 13.8863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200091_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 200091_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:32:19.94 -29:18:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.747 5644053533417422976 128.08291317593 -29.31179946892 14.1371 14.0632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200225_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 200225_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:35:55.38 -27:24:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.477 5646569422181781888 128.98032421227 -27.41028624322 14.2778 13.9562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200289_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 200289_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:50:02.22 -26:04:43.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200299_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 200299_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:33:56.66 -27:32:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200366_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 200366_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:35:09.72 -28:22:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.982 5645659370152371968 128.78955936329 -28.36930933870 14.2810 13.7686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 40269_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 40269_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:19:05.24 -24:02:13.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61781_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 61781_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:42.82 -25:14:44.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100249_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
Preparing report for the candidate 100249_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34846_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 34846_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:42.81 -23:37:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120332_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 120332_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:33:02.87 -29:51:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164289_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 164289_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:41.23 -29:42:57.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136310_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 136310_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:18.51 -28:30:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45596_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 45596_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:24:26.00 -24:21:24.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11914_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013
The candidate 11914_fd_Pyx-01-Q2b1x1_2026-04-08_21-13-01_20.00sec_-5.00C_LIGHT_0013 did not pass the final checks
**** FOUND 08:31:01.45 -21:47:37.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 251s
make_report_in_HTML.sh TOTAL: 1123s
Prepared the HTML report for the field Pyx-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:38:12.83 -22:51:58.4
08:45:57.98 -29:45:07.4
08:47:30.57 -23:52:02.1
08:41:09.81 -27:43:26.5
08:43:54.65 -24:39:09.4
08:38:05.06 -28:19:24.8
08:50:05.29 -26:41:15.4
08:28:12.84 -28:30:43.7
08:43:57.43 -28:01:22.0
08:41:02.43 -30:10:10.3
08:48:19.76 -28:30:09.2
08:21:53.70 -27:09:00.2
08:48:53.47 -27:28:16.3
08:41:37.39 -27:32:52.3
08:45:11.39 -24:26:08.1
08:53:49.32 -28:48:29.5
08:48:51.46 -27:32:58.1
08:25:53.78 -24:34:08.2
08:48:15.21 -28:08:57.3
08:20:41.84 -28:36:31.0
08:24:31.35 -27:57:00.9
08:59:19.52 -29:15:21.6
08:40:39.63 -24:10:29.5
08:55:23.57 -27:20:18.3
08:39:29.10 -27:26:02.2
08:47:33.41 -28:27:12.7
08:56:38.90 -21:49:44.0
08:39:14.57 -27:19:28.5
08:18:57.32 -27:36:47.0
08:19:27.30 -25:13:32.2
08:57:27.73 -24:09:31.4
08:45:23.45 -25:58:26.1
08:36:27.36 -30:02:07.7
08:38:28.14 -29:41:03.8
08:22:39.68 -27:35:11.3
08:25:28.57 -29:29:35.1
08:50:55.71 -28:23:51.7
08:29:30.75 -27:33:30.0
08:42:08.13 -27:43:12.7
08:53:23.12 -28:21:04.3
08:36:58.45 -26:36:59.3
08:49:43.62 -27:35:38.7
08:49:48.30 -22:43:06.8
########### Completed Pyx-01-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 ####
08:38:12.83 -22:51:58.4
08:47:30.57 -23:52:02.1
08:41:09.81 -27:43:26.5
08:43:54.65 -24:39:09.4
08:38:05.06 -28:19:24.8
08:50:05.29 -26:41:15.4
08:28:12.84 -28:30:43.7
08:43:57.43 -28:01:22.0
08:41:02.43 -30:10:10.3
08:48:19.76 -28:30:09.2
08:21:53.70 -27:09:00.2
08:48:53.47 -27:28:16.3
08:41:37.39 -27:32:52.3
08:45:11.39 -24:26:08.1
08:53:49.32 -28:48:29.5
08:48:51.46 -27:32:58.1
08:25:53.78 -24:34:08.2
08:48:15.21 -28:08:57.3
08:20:41.84 -28:36:31.0
08:24:31.35 -27:57:00.9
08:59:19.52 -29:15:21.6
08:40:39.63 -24:10:29.5
08:55:23.57 -27:20:18.3
08:39:29.10 -27:26:02.2
08:47:33.41 -28:27:12.7
08:56:38.90 -21:49:44.0
08:39:14.57 -27:19:28.5
08:18:57.32 -27:36:47.0
08:19:27.30 -25:13:32.2
08:57:27.73 -24:09:31.4
08:45:23.45 -25:58:26.1
08:36:27.36 -30:02:07.7
08:38:28.14 -29:41:03.8
08:22:39.68 -27:35:11.3
08:25:28.57 -29:29:35.1
08:50:55.71 -28:23:51.7
08:29:30.75 -27:33:30.0
08:42:08.13 -27:43:12.7
08:53:23.12 -28:21:04.3
08:36:58.45 -26:36:59.3
08:49:43.62 -27:35:38.7
08:49:48.30 -22:43:06.8
08:45:57.98 -29:45:07.4
###################################################################################
08:38:12.83 -22:51:58.4 -- not an asteroid (will add it to exclusion list)
08:47:30.57 -23:52:02.1 -- not an asteroid (will add it to exclusion list)
08:41:09.81 -27:43:26.5 -- not an asteroid (will add it to exclusion list)
08:43:54.65 -24:39:09.4 -- not an asteroid (will add it to exclusion list)
08:38:05.06 -28:19:24.8 -- not an asteroid (will add it to exclusion list)
08:50:05.29 -26:41:15.4 -- not an asteroid (will add it to exclusion list)
08:28:12.84 -28:30:43.7 -- not an asteroid (will add it to exclusion list)
08:43:57.43 -28:01:22.0 -- not an asteroid (will add it to exclusion list)
08:41:02.43 -30:10:10.3 -- not an asteroid (will add it to exclusion list)
08:48:19.76 -28:30:09.2 -- not an asteroid (will add it to exclusion list)
08:21:53.70 -27:09:00.2 -- not an asteroid (will add it to exclusion list)
08:48:53.47 -27:28:16.3 -- not an asteroid (will add it to exclusion list)
08:41:37.39 -27:32:52.3 -- not an asteroid (will add it to exclusion list)
08:45:11.39 -24:26:08.1 -- not an asteroid (will add it to exclusion list)
08:53:49.32 -28:48:29.5 -- not an asteroid (will add it to exclusion list)
08:48:51.46 -27:32:58.1 -- not an asteroid (will add it to exclusion list)
08:25:53.78 -24:34:08.2 -- not an asteroid (will add it to exclusion list)
08:48:15.21 -28:08:57.3 -- not an asteroid (will add it to exclusion list)
08:20:41.84 -28:36:31.0 -- not an asteroid (will add it to exclusion list)
08:24:31.35 -27:57:00.9 -- not an asteroid (will add it to exclusion list)
08:59:19.52 -29:15:21.6 -- not an asteroid (will add it to exclusion list)
08:40:39.63 -24:10:29.5 -- not an asteroid (will add it to exclusion list)
08:55:23.57 -27:20:18.3 -- not an asteroid (will add it to exclusion list)
08:39:29.10 -27:26:02.2 -- not an asteroid (will add it to exclusion list)
08:47:33.41 -28:27:12.7 -- not an asteroid (will add it to exclusion list)
08:56:38.90 -21:49:44.0 -- not an asteroid (will add it to exclusion list)
08:39:14.57 -27:19:28.5 -- not an asteroid (will add it to exclusion list)
08:18:57.32 -27:36:47.0 -- not an asteroid (will add it to exclusion list)
08:19:27.30 -25:13:32.2 -- not an asteroid (will add it to exclusion list)
08:57:27.73 -24:09:31.4 -- not an asteroid (will add it to exclusion list)
08:45:23.45 -25:58:26.1 -- not an asteroid (will add it to exclusion list)
08:36:27.36 -30:02:07.7 -- not an asteroid (will add it to exclusion list)
08:38:28.14 -29:41:03.8 -- not an asteroid (will add it to exclusion list)
08:22:39.68 -27:35:11.3 -- not an asteroid (will add it to exclusion list)
08:25:28.57 -29:29:35.1 -- not an asteroid (will add it to exclusion list)
08:50:55.71 -28:23:51.7 -- not an asteroid (will add it to exclusion list)
08:29:30.75 -27:33:30.0 -- not an asteroid (will add it to exclusion list)
08:42:08.13 -27:43:12.7 -- not an asteroid (will add it to exclusion list)
08:53:23.12 -28:21:04.3 -- not an asteroid (will add it to exclusion list)
08:36:58.45 -26:36:59.3 -- not an asteroid (will add it to exclusion list)
08:49:43.62 -27:35:38.7 -- not an asteroid (will add it to exclusion list)
08:49:48.30 -22:43:06.8 -- not an asteroid (will add it to exclusion list)
08:45:57.98 -29:45:07.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
08:18:57.32 -27:36:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:19:27.30 -25:13:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:20:41.84 -28:36:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:21:53.70 -27:09:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:22:39.68 -27:35:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:31.35 -27:57:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:28.57 -29:29:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:25:53.78 -24:34:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:28:12.84 -28:30:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:30.75 -27:33:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:36:27.36 -30:02:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:36:58.45 -26:36:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:38:05.06 -28:19:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:38:12.83 -22:51:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:38:28.14 -29:41:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:39:14.57 -27:19:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:39:29.10 -27:26:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:39.63 -24:10:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:41:02.43 -30:10:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:41:09.81 -27:43:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:41:37.39 -27:32:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:42:08.13 -27:43:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:43:54.65 -24:39:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:43:57.43 -28:01:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:45:11.39 -24:26:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:45:23.45 -25:58:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:45:57.98 -29:45:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:47:30.57 -23:52:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:47:33.41 -28:27:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:15.21 -28:08:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:19.76 -28:30:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:51.46 -27:32:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:53.47 -27:28:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:49:43.62 -27:35:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:49:48.30 -22:43:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:50:05.29 -26:41:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:50:55.71 -28:23:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:53:23.12 -28:21:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:53:49.32 -28:48:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:55:23.57 -27:20:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:56:38.90 -21:49:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:57:27.73 -24:09:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:59:19.52 -29:15:21.6 -- 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)
08:18:57.32 -27:36:47.0 -- not a known variable star
08:19:27.30 -25:13:32.2 -- not a known variable star
08:20:41.84 -28:36:31.0 -- not a known variable star
08:21:53.70 -27:09:00.2 -- a known variable star
08:22:39.68 -27:35:11.3 -- not a known variable star
08:24:31.35 -27:57:00.9 -- a known variable star
08:25:28.57 -29:29:35.1 -- a known variable star
08:25:53.78 -24:34:08.2 -- not a known variable star
08:28:12.84 -28:30:43.7 -- not a known variable star
08:29:30.75 -27:33:30.0 -- not a known variable star
08:36:27.36 -30:02:07.7 -- not a known variable star
08:36:58.45 -26:36:59.3 -- a known variable star
08:38:05.06 -28:19:24.8 -- a known variable star
08:38:12.83 -22:51:58.4 -- a known variable star
08:38:28.14 -29:41:03.8 -- a known variable star
08:39:14.57 -27:19:28.5 -- not a known variable star
08:39:29.10 -27:26:02.2 -- not a known variable star
08:40:39.63 -24:10:29.5 -- not a known variable star
08:41:02.43 -30:10:10.3 -- not a known variable star
08:41:09.81 -27:43:26.5 -- not a known variable star
08:41:37.39 -27:32:52.3 -- not a known variable star
08:42:08.13 -27:43:12.7 -- not a known variable star
08:43:54.65 -24:39:09.4 -- not a known variable star
08:43:57.43 -28:01:22.0 -- not a known variable star
08:45:11.39 -24:26:08.1 -- not a known variable star
08:45:23.45 -25:58:26.1 -- not a known variable star
08:45:57.98 -29:45:07.4 -- a known variable star
08:47:30.57 -23:52:02.1 -- not a known variable star
08:47:33.41 -28:27:12.7 -- not a known variable star
08:48:15.21 -28:08:57.3 -- not a known variable star
08:48:19.76 -28:30:09.2 -- not a known variable star
08:48:51.46 -27:32:58.1 -- not a known variable star
08:48:53.47 -27:28:16.3 -- not a known variable star
08:49:43.62 -27:35:38.7 -- a known variable star
08:49:48.30 -22:43:06.8 -- not a known variable star
08:50:05.29 -26:41:15.4 -- not a known variable star
08:50:55.71 -28:23:51.7 -- not a known variable star
08:53:23.12 -28:21:04.3 -- a known variable star
08:53:49.32 -28:48:29.5 -- not a known variable star
08:55:23.57 -27:20:18.3 -- a known variable star
08:56:38.90 -21:49:44.0 -- not a known variable star
08:57:27.73 -24:09:31.4 -- a known variable star
08:59:19.52 -29:15:21.6 -- not a known variable star
Found 31 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
43 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 43 (excluding asteroids and hot pixels, 31 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461139.59186795 -observatory V36
23:33:08.85 -05:22:01.0 Mercury (0.2mag)
02:35:15.96 +15:05:59.4 Venus (-3.9mag)
23:58:10.90 -01:18:00.7 Mars (1.2mag)
07:09:45.11 +22:50:50.4 Jupiter (-2.1mag)
00:26:04.60 +00:29:31.7 Saturn (0.9mag)
03:46:17.18 +19:42:55.7 Uranus (5.8mag)
00:09:55.34 -00:21:10.5 Neptune (7.8mag)
20:33:24.46 -22:52:27.0 Pluto (14.5mag)
18:31:33.37 -27:54:08.5 Moon (-10.7mag)
-rw-r--r-- 1 apache apache 362 Apr 8 21:35 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461139.59186795:
07:09:47.82 +22:50:47.4 Io (5.7mag)
07:09:52.17 +22:50:38.3 Europa (5.9mag)
07:10:00.84 +22:50:13.9 Ganymede (5.3mag)
07:09:14.02 +22:51:55.9 Callisto (6.5mag)
07:13:22.07 +22:41:50.2 Himalia (15.3mag)
07:09:48.95 +22:50:43.4 Thebe (16.2mag)
07:13:23.99 +23:11:11.1 Elara (17.3mag)
07:08:09.76 +23:34:27.7 Pasiphae (17.4mag)
07:18:13.55 +22:48:07.5 Carme (18.5mag)
00:26:10.99 +00:29:20.9 Titan (8.8mag)
00:26:09.64 +00:29:39.6 Rhea (10.1mag)
00:25:58.55 +00:30:43.6 Iapetus (11.5mag)
00:26:15.77 +00:29:17.9 Hyperion (14.8mag)
00:27:46.76 +00:39:03.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 8 21:35 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.59186795:
15:04:09.22 -10:52:33.2 JWST
17:25:35.39 +39:57:40.4 Chandra
16:26:19.12 -55:07:48.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 8 21:35 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.59186795 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:45.28 -28:23:21.3 13.9mag P/2010 H2 (Vales)
05:01:57.71 -69:59:58.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:04.16 +31:23:35.0 17.2mag C/2017 K2 (PANSTARRS)
17:30:53.74 +09:43:16.4 17.6mag C/2021 G2 (ATLAS)
23:08:15.42 +28:58:05.3 17.0mag C/2022 E2 (ATLAS)
04:21:16.41 +25:50:49.5 15.9mag C/2022 N2 (PANSTARRS)
09:02:12.18 +31:57:05.8 16.2mag C/2022 QE78 (ATLAS)
08:30:12.85 -00:54:16.2 17.3mag C/2022 R6 (PANSTARRS)
18:55:08.62 +17:56:42.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:45.09 -11:37:14.8 17.6mag P/2023 B1 (PANSTARRS)
09:11:09.06 -13:00:49.9 17.6mag C/2023 F3 (ATLAS)
21:46:50.77 +62:31:13.2 17.5mag C/2023 H5 (Lemmon)
19:24:33.00 -03:38:15.2 14.2mag C/2023 R1 (PANSTARRS)
21:41:20.73 +84:58:48.7 17.8mag C/2023 X2 (Lemmon)
06:15:15.00 +63:33:26.1 17.1mag C/2024 A1 (ATLAS)
04:57:54.85 +15:46:54.3 10.6mag C/2024 E1 (Wierzchos)
16:23:29.43 +05:15:17.8 17.4mag C/2024 G6 (ATLAS)
20:18:37.47 +13:25:58.6 14.7mag C/2024 J3 (ATLAS)
03:20:15.68 -23:27:30.9 16.4mag C/2024 T5 (ATLAS)
05:10:59.79 +47:03:27.4 17.7mag C/2025 J1 (Borisov)
14:07:26.47 +40:09:45.4 14.9mag C/2025 L1 (ATLAS)
03:14:38.52 -25:10:02.0 17.8mag C/2025 Q3 (ATLAS)
23:02:29.85 +19:46:34.7 9.6mag C/2025 R3 (PANSTARRS)
12:57:07.72 +02:34:50.2 17.5mag C/2025 Y1 (ATLAS)
02:16:12.09 +03:45:13.7 10.3mag C/2026 A1 (MAPS)
23:39:31.60 +35:52:04.3 14.4mag C/2026 B2 (Sun-Gao)
18:29:27.57 -10:04:39.7 12.2mag 10P/Tempel
15:09:22.92 +03:52:15.8 13.4mag 24P/Schaumasse
11:04:49.16 -01:45:34.4 15.7mag 29P/Schwassmann-Wachmann
17:58:18.45 -09:52:32.2 17.8mag 40P/Vaisala
10:38:17.43 -04:40:55.6 16.8mag 43P/Wolf-Harrington
01:38:00.42 +16:18:02.8 17.2mag 47P/Ashbrook-Jackson
06:58:19.61 +38:28:41.8 17.0mag 63P/Wild
23:20:07.83 -12:17:35.9 15.7mag 65P/Gunn
03:45:05.55 +18:48:37.5 15.9mag 76P/West-Kohoutek-Ikemura
00:50:23.36 +06:51:46.9 14.4mag 78P/Gehrels
22:41:43.31 -11:25:35.7 14.6mag 88P/Howell
01:51:05.94 +18:45:41.6 15.1mag 93P/Lovas
04:42:04.14 +31:54:06.3 16.3mag 123P/West-Hartley
08:20:45.02 +41:33:06.2 16.2mag 124P/Mrkos
02:22:36.78 +13:35:25.0 16.4mag 128P/Shoemaker-Holt
02:34:01.87 +13:37:47.6 17.5mag 131P/Mueller
00:50:26.47 +10:43:48.8 11.0mag 141P/Machholz
01:00:11.08 +02:16:46.4 11.0mag 141P-A/Machholz
23:49:04.78 -01:30:16.1 13.7mag 141P-D/Machholz
01:29:44.91 +03:59:14.3 17.9mag 141P-I/Machholz
00:43:09.98 -04:58:58.6 15.2mag 162P/SidingSpring
10:30:07.48 +31:19:31.3 17.9mag 164P/Christensen
06:23:44.87 +24:27:05.6 17.9mag 198P/ODAS
15:03:40.33 -00:50:18.0 17.4mag 210P/Christensen
21:18:06.82 -13:07:13.4 17.5mag 218P/LINEAR
17:14:06.70 -14:44:45.4 16.2mag 235P/LINEAR
05:19:43.73 +34:07:41.7 16.6mag 240P/NEAT
07:35:20.87 -05:56:34.8 17.7mag 242P/Spahr
15:45:05.35 +06:31:03.2 17.5mag 391P/Kowalski
07:31:46.47 +21:19:59.8 17.6mag 450P/LONEOS
05:25:57.44 +45:26:20.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 8 21:35 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -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
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
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
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -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
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
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
-rw-r--r-- 1 apache apache 5.8K Apr 8 21:35 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 8 21:35 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:05:53.820 +48:45:26.80 AT 2026ifh 2026-03-23.81 21.26
16:27:03.110 +44:45:26.84 AT 2026ifg 2026-03-23.81 21.9
16:41:17.580 +44:27:03.47 AT 2026iff 2026-03-23.81 22.17
16:30:53.670 +55:47:08.39 AT 2026ife 2026-03-30.85 20.99
16:07:35.060 +52:45:21.40 AT 2026ifd 2026-03-30.82 20.79
12:49:57.980 +19:52:49.93 AT 2026ifc 2026-03-20.70 19.71
15:58:08.890 +36:23:36.27 AT 2026ifb 2026-03-18.81 20.34
15:47:02.670 +48:09:28.72 AT 2026ifa 2026-03-30.81 20.31
15:30:58.600 +53:17:16.37 AT 2026iez 2026-03-23.80 21.21
10:25:53.600 +03:15:54.45 AT 2026iey 2026-03-24.63 22.18
19:10:17.892 -22:37:27.97 AT 2026iex 2026-03-30.80 18.87
12:44:39.935 -44:03:37.93 AT 2026iew 2026-03-31.50 19.02
14:52:16.530 -15:21:39.90 AT 2026iev 2026-04-02.23 19.3
17:43:01.293 -27:00:33.19 AT 2026ieu 2026-04-04.35 19.44
16:55:57.478 +11:06:09.42 AT 2026iet 2026-04-04.38 19.2385
16:23:37.422 +39:12:11.82 AT 2026ies 2026-04-04.41 19.2599
03:56:10.038 -48:29:05.29 AT 2026ier 2026-01-17.17 23.94
16:57:33.187 +32:51:43.01 AT 2026ieq 2026-03-31.41 18.7085
10:09:46.469 -39:37:05.37 AT 2026iep 2026-03-28.44 19.36
19:10:06.552 -14:29:45.88 AT 2026ieo 2026-03-25.79 19.76
-rw-r--r-- 1 apache apache 30K Apr 8 21:35 tns_transients_list.txt
