This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107171584665401984,2461135.6385,13.16,0.05,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
Gaia DR3 3107171584665401984 20260405.1385 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119460486829616640,2461135.6385,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119460486829616640 20260405.1385 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106045203719510272,2461135.6385,13.01,0.05,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
Gaia DR3 3106045203719510272 20260405.1385 13.01CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107274358943072000,2461135.6385,12.54,0.05,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
Gaia DR3 3107274358943072000 20260405.1385 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101673034391323264,2461135.6385,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101673034391323264 20260405.1385 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064143.42-010627.5,2461135.6385,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064143.42-010627.5 20260405.1385 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5760-05.4530,2461135.6385,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.5760-05.4530 20260405.1385 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1385 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107197805444320128,2461135.6385,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107197805444320128 20260405.1385 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125569957548660864,2461135.6385,12.35,0.05,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 3125569957548660864 20260405.1385 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1385 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.30,0.05,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 20260405.1385 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125681313161965056,2461135.6385,12.26,0.05,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 3125681313161965056 20260405.1385 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 12569794,2461135.6385,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12569794 20260405.1385 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6522-00.6011,2461135.6385,11.63,0.05,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 J103.6522-00.6011 20260405.1385 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125658296436103552,2461135.6385,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125658296436103552 20260405.1385 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065134.58+002720.2,2461135.6385,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065134.58+002720.2 20260405.1385 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113144097467624576,2461135.6385,10.96,0.05,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 3113144097467624576 20260405.1385 10.96CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113577274989419904,2461135.6385,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113577274989419904 20260405.1385 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105345059631344768,2461135.6385,11.91,0.05,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 3105345059631344768 20260405.1385 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106324999372001664,2461135.6385,12.16,0.05,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
Gaia DR3 3106324999372001664 20260405.1385 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100480579673234176,2461135.6385,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100480579673234176 20260405.1385 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.2775-01.0440,2461135.6385,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.2775-01.0440 20260405.1385 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101049125963883520,2461135.6385,12.15,0.05,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
Gaia DR3 3101049125963883520 20260405.1385 12.15CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125504223071142784,2461135.6385,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125504223071142784 20260405.1385 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.3878-01.3922,2461135.6385,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.3878-01.3922 20260405.1385 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103981287255761536,2461135.6385,12.24,0.05,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 3103981287255761536 20260405.1385 12.24CV 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
Mean magnitude and position on the discovery images:
2026 04 05.1385 2461135.6385 12.34 06:48:16.68 -01:48:39.5
214.18391 -1.52852 galactic Mon Second-epoch detections are separated by 0.7" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3106310087243820928 | 06:48:16.68 -01:48:39.5 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: F4V 2012A&A...543A.125G CoRoT 102889617
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3106310087243820928,2461135.6385,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3106310087243820928 20260405.1385 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.35,0.05,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 20260405.1385 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113610294697190784,2461135.6385,12.49,0.05,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
Gaia DR3 3113610294697190784 20260405.1385 12.49CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3104037190549906304,2461135.6385,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3104037190549906304 20260405.1385 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1385 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9551+00.2304,2461135.6385,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9551+00.2304 20260405.1385 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101886477089103232,2461135.6385,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101886477089103232 20260405.1385 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106082209159437440,2461135.6385,12.42,0.05,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 3106082209159437440 20260405.1385 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9976-01.1014,2461135.6385,12.63,0.05,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 J101.9976-01.1014 20260405.1385 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113466018154637184,2461135.6385,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113466018154637184 20260405.1385 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101684166946863104,2461135.6385,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101684166946863104 20260405.1385 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125521647757070208,2461135.6385,12.65,0.05,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 3125521647757070208 20260405.1385 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.68,0.05,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 20260405.1385 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0649315-012934,2461135.6385,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0649315-012934 20260405.1385 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106053763595735040,2461135.6385,12.74,0.05,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
Gaia DR3 3106053763595735040 20260405.1385 12.74CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461135.6385,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102785122 20260405.1385 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.77,0.05,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 20260405.1385 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1385 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113470691079092224,2461135.6385,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113470691079092224 20260405.1385 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6385,11.86,0.05,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 20260405.1385 11.86CV 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461135.63875604 05.04.2026 03:19:38.522 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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): 29722
Objects passed selection criteria: 29600
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: 21964
Average stars matched: 20793.8 (94.672 %)
Memory usage VmPeak: 133180 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 4 22:23:32 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461135.63875604 05.04.2026 03:19:38.522 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 347
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 97 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): 216750
Objects passed selection criteria: 216196
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: 170731
Average stars matched: 160417 (93.9586 %)
Memory usage VmPeak: 2162664 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 4 22:28:19 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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: 2461135.63815995
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:35.471 -01:57:47.15
Angular distance between the image centers 0.0523 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:37.561 -01:57:44.87
Angular distance between the image centers 0.0481 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 06:51:35.471 -01:57:47.15
Second-epoch second image center 06:51:37.561 -01:57:44.87
Angular distance between the image centers 0.00873 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.mFSlSKI6qS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.14vwG1dgtV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits &> /tmp/tmp.Bn3kvkm4qs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits &> /tmp/tmp.o0d3GmE1kA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
14.1 mag. fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (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.mFSlSKI6qS (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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
WARNING: Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.14vwG1dgtV (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/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Bn3kvkm4qs (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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1149, passed=15562
Got 15562 stars (including 14398 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 15562 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 413 to 468 (Dec -7.3 to 3.4)
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...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 15227 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 15227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 15226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 931 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_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.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.o0d3GmE1kA (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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1226, passed=17077
Got 17077 stars (including 15835 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 17077 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 917.3'
Seting catalog search parameters based on the expected field of view 917.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012740 (45.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010192 (36.7 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 659 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 607 matched stars entering correct_measured_positions(), 561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.21"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 604 matched stars entering correct_measured_positions(), 9350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.52"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 700 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 672 matched stars entering correct_measured_positions(), 9389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
WARNING: Accuracy estimation diagnostic: 671 matched stars entering correct_measured_positions(), 10591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.78"
Excluding outliers - 671 stars left (next iteration limit 664)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out54229.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53096_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 53096_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (286.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54229_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 54229_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:24.44 -00:31:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.345 3113209110392080384 102.10191212973 -00.52416580695 11.6927 11.3805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:35.471 -01:57:47.15
Angular distance between the image centers 0.0523 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:37.561 -01:57:44.87
Angular distance between the image centers 0.0481 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 06:51:35.471 -01:57:47.15
Second-epoch second image center 06:51:37.561 -01:57:44.87
Angular distance between the image centers 0.00873 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.x9tqordKFk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.sbbtsz4DcG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits &> /tmp/tmp.Tfzf5GqGyZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits &> /tmp/tmp.5HVI5gKeum
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 289 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.2 mag. fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
13.3 mag. fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.x9tqordKFk (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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
WARNING: Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.sbbtsz4DcG (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/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Tfzf5GqGyZ (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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=12858, passed=129031
Got 129031 stars (including 116011 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 129031 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 126849 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 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 126849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
WARNING: Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 126816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 928 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_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.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.5HVI5gKeum (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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=14331, passed=136363
Got 136363 stars (including 121891 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 136363 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 917.3'
Seting catalog search parameters based on the expected field of view 917.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012740 (45.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010192 (36.7 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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 652 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 595 matched stars entering correct_measured_positions(), 548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 593 matched stars entering correct_measured_positions(), 72576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.64"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 693 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 657 matched stars entering correct_measured_positions(), 72601 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.63"
WARNING: Accuracy estimation diagnostic: 657 matched stars entering correct_measured_positions(), 82948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.92"
Excluding outliers - 657 stars left (next iteration limit 652)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-18-47_20.00sec_-5.00C_LIGHT_0020.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.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_2026-04-04_CI_Mon-02-Q2b1x1_222105_TTUQ2b1x1_32638_w4UbG2e9/wcs_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out285102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out285419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out295281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out296975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out297680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out298320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out302460.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out285080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out285438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out295741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out296805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out297886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67235.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 65s
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: 34s
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Considering the candidate 285079_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285079_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (160.0") between the two second-epoch detections
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Considering the candidate 285080_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285080_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285084_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285084_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 285094_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285094_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (326.2") between the two second-epoch detections
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Considering the candidate 285099_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285099_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (45.2") between the two second-epoch detections
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Considering the candidate 285100_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285100_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 285102_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285102_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:11.64 -02:02:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.917 3106617259003491456 100.79850991076 -02.03450460142 13.7064 13.1691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285106_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285106_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:09.68 -03:21:54.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 285111_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285111_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:47.26 -05:59:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.541 3100397669625141504 101.44666535656 -05.99579212220 13.4065 12.3822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285117_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285117_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (355.4") between the two second-epoch detections
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Considering the candidate 285118_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285118_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (117.2") between the two second-epoch detections
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Considering the candidate 285120_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285120_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285129_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285129_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (73.3") between the two second-epoch detections
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Considering the candidate 285135_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285135_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:04.69 +01:03:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.659 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285140_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285140_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 285144_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285144_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285158_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285158_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:48.53 -03:18:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.372 3102817832155590400 103.45189812196 -03.31686080716 13.6976 12.7865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285162_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285162_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:38.01 +00:05:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.169 3119509685677083136 100.90815124971 +00.09182959907 13.7914 13.3091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285165_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285165_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (397.3") between the two second-epoch detections
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Considering the candidate 285167_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285167_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (404.8") between the two second-epoch detections
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Considering the candidate 285173_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285173_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (481.9") between the two second-epoch detections
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Considering the candidate 285174_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285174_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (128.4") between the two second-epoch detections
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Considering the candidate 285176_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285176_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (271.2") between the two second-epoch detections
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Considering the candidate 285194_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285194_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285195_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285195_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (64.3") between the two second-epoch detections
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Considering the candidate 285197_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285197_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (241.8") between the two second-epoch detections
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Considering the candidate 285200_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285200_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (363.6") between the two second-epoch detections
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Considering the candidate 285201_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285201_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (64.7") between the two second-epoch detections
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Considering the candidate 285203_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285203_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:23.77 -05:15:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 1.364 3101964366313335296 102.59896228734 -05.26153723479 13.5496 13.0347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285207_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285207_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:52.34 -02:40:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.357 3105924708418102400 102.46800809269 -02.67331367872 13.2790 12.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285208_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285208_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285217_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285217_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (310.8") between the two second-epoch detections
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Considering the candidate 285218_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285218_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (184.9") between the two second-epoch detections
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Considering the candidate 285222_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285222_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (60.5") between the two second-epoch detections
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Considering the candidate 285225_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285225_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285226_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285226_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (273.9") between the two second-epoch detections
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Considering the candidate 285228_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285228_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (377.5") between the two second-epoch detections
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Considering the candidate 285229_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285229_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285237_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285237_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (240.3") between the two second-epoch detections
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Considering the candidate 285238_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285238_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (94.8") between the two second-epoch detections
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Considering the candidate 285240_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285240_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (382.2") between the two second-epoch detections
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Considering the candidate 285242_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285242_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (414.0") between the two second-epoch detections
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Considering the candidate 285243_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285243_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (91.3") between the two second-epoch detections
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Considering the candidate 285244_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285244_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (242.8") between the two second-epoch detections
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Considering the candidate 285245_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285245_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (185.2") between the two second-epoch detections
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Considering the candidate 285255_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285255_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (85.9") between the two second-epoch detections
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Considering the candidate 285262_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285262_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:31:35.33 -06:17:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.136 3103272548931943680 097.89738469210 -06.29330208244 13.1214 12.5797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285263_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285263_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (73.6") between the two second-epoch detections
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Considering the candidate 285265_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285265_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (347.6") between the two second-epoch detections
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Considering the candidate 285268_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285268_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:55:04.91 -01:02:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.744 3112333899136721408 103.77089108376 -01.04932192669 13.4551 12.7464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285272_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285272_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (272.8") between the two second-epoch detections
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Considering the candidate 285274_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285274_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285284_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285284_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:09.69 -03:38:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.927 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285285_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285285_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (157.6") between the two second-epoch detections
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Considering the candidate 285286_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285286_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285296_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285296_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (466.6") between the two second-epoch detections
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Considering the candidate 285298_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285298_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285299_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285299_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285300_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285300_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (420.1") between the two second-epoch detections
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Considering the candidate 285304_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285304_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (105.5") between the two second-epoch detections
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Considering the candidate 285307_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285307_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (569.5") between the two second-epoch detections
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Considering the candidate 285309_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285309_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (430.9") between the two second-epoch detections
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Considering the candidate 285314_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285314_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (71.8") between the two second-epoch detections
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Considering the candidate 285317_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285317_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (461.0") between the two second-epoch detections
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Considering the candidate 285318_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285318_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (338.5") between the two second-epoch detections
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Considering the candidate 285320_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285320_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:45.17 -01:18:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.045 3107234982682679808 100.43805540528 -01.31615820583 13.1525 12.7239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285321_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285321_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285322_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285322_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (107.5") between the two second-epoch detections
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Considering the candidate 285327_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285327_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (687.8") between the two second-epoch detections
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Considering the candidate 285329_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285329_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (708.2") between the two second-epoch detections
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Considering the candidate 285333_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285333_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (290.5") between the two second-epoch detections
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Considering the candidate 285335_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285335_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (551.9") between the two second-epoch detections
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Considering the candidate 285336_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285336_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (58.0") between the two second-epoch detections
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Considering the candidate 285337_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285337_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285344_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285344_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (538.0") between the two second-epoch detections
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Considering the candidate 285345_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285345_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (70.9") between the two second-epoch detections
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Considering the candidate 285348_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285348_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (129.7") between the two second-epoch detections
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Considering the candidate 285350_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285350_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (233.7") between the two second-epoch detections
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Considering the candidate 285355_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285355_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:55.94 -05:49:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285358_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285358_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (563.2") between the two second-epoch detections
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Considering the candidate 285360_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285360_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (694.4") between the two second-epoch detections
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Considering the candidate 285361_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285361_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (114.7") between the two second-epoch detections
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Considering the candidate 285363_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285363_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (489.4") between the two second-epoch detections
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Considering the candidate 285367_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285367_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (261.1") between the two second-epoch detections
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Considering the candidate 285368_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285368_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (222.8") between the two second-epoch detections
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Considering the candidate 285370_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285370_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:13.47 -00:19:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285371_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285371_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:30:20.41 -01:44:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 3.808 3117526926911357056 097.58401220574 -01.74888400398 12.0708 10.6232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285373_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285373_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (125.5") between the two second-epoch detections
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Considering the candidate 285376_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285376_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 285377_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285377_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (330.7") between the two second-epoch detections
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Considering the candidate 285379_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285379_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:08.07 -05:53:00.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 285380_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285380_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (224.3") between the two second-epoch detections
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Considering the candidate 285381_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285381_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (74.9") between the two second-epoch detections
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Considering the candidate 285382_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285382_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (243.4") between the two second-epoch detections
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Considering the candidate 285383_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285383_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (62.3") between the two second-epoch detections
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Considering the candidate 285384_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285384_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (307.8") between the two second-epoch detections
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Considering the candidate 285387_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285387_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (125.6") between the two second-epoch detections
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Considering the candidate 285393_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285393_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:02.39 +01:07:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285395_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285395_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (395.4") between the two second-epoch detections
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Considering the candidate 285398_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285398_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (429.4") between the two second-epoch detections
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Considering the candidate 285400_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285400_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:39.56 -01:31:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 2.783 3106905262331173632 099.66491829980 -01.52429610039 12.4571 11.4111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285403_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285403_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285406_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285406_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (538.1") between the two second-epoch detections
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Considering the candidate 285410_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285410_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (254.8") between the two second-epoch detections
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Considering the candidate 285413_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285413_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285414_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285414_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (65.1") between the two second-epoch detections
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Considering the candidate 285415_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285415_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (48.7") between the two second-epoch detections
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Considering the candidate 285416_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285416_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (360.1") between the two second-epoch detections
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Considering the candidate 285419_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285419_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:25.97 -04:51:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 1.462 3102225057948914176 101.35791455966 -04.86586500739 12.0278 11.0816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 285420_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285420_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (585.4") between the two second-epoch detections
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Considering the candidate 285424_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285424_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:11.51 -01:33:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285427_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285427_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (404.0") between the two second-epoch detections
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Considering the candidate 285428_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285428_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (197.5") between the two second-epoch detections
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Considering the candidate 285429_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285429_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (282.4") between the two second-epoch detections
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Considering the candidate 285431_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285431_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (177.8") between the two second-epoch detections
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Considering the candidate 285432_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285432_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (276.2") between the two second-epoch detections
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Considering the candidate 285434_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285434_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (338.9") between the two second-epoch detections
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Considering the candidate 285435_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285435_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285436_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285436_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (628.5") between the two second-epoch detections
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Considering the candidate 285438_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 285438_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 285439_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285439_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:44.44 +00:29:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285442_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285442_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (386.7") between the two second-epoch detections
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Considering the candidate 285444_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 285444_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (155.5") between the two second-epoch detections
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Considering the candidate 287246_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 287246_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:40.20 -00:32:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288018_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 288018_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:37.28 +00:26:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288432_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 288432_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:39.80 +00:25:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288706_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 288706_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 289163_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 289163_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:37.75 +00:43:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289589_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 289589_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (434.6") between the two second-epoch detections
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Considering the candidate 289960_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 289960_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (140.0") between the two second-epoch detections
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Considering the candidate 290016_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 290016_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:30.50 -01:04:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290134_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 290134_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:41.65 -00:33:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290522_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 290522_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (39.9") between the two second-epoch detections
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Considering the candidate 291272_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 291272_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:36:41.02 -05:13:19.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291561_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 291561_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (534.7") between the two second-epoch detections
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Considering the candidate 291690_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 291690_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (332.8") between the two second-epoch detections
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Considering the candidate 291901_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 291901_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (184.8") between the two second-epoch detections
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Considering the candidate 292115_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 292115_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (63.7") between the two second-epoch detections
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Considering the candidate 292493_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 292493_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:44.49 -00:31:38.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 292930_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 292930_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (228.7") between the two second-epoch detections
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Considering the candidate 292965_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 292965_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (63.5") between the two second-epoch detections
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Considering the candidate 293194_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 293194_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (502.8") between the two second-epoch detections
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Considering the candidate 293267_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 293267_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (570.5") between the two second-epoch detections
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Considering the candidate 293299_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 293299_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 293762_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 293762_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (71.6") between the two second-epoch detections
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Considering the candidate 293818_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 293818_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:09.28 -05:52:26.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293996_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 293996_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:08.13 -04:35:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294055_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294055_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (48.6") between the two second-epoch detections
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Considering the candidate 294240_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 294240_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 294246_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294246_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (95.6") between the two second-epoch detections
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Considering the candidate 294329_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294329_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (86.3") between the two second-epoch detections
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Considering the candidate 294441_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294441_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:44.59 -04:35:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294515_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294515_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (147.7") between the two second-epoch detections
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Considering the candidate 294570_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294570_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (528.3") between the two second-epoch detections
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Considering the candidate 294703_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294703_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (227.7") between the two second-epoch detections
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Considering the candidate 294997_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 294997_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:16.41 -04:45:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295003_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295003_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:28.95 -00:00:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295019_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295019_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:49.14 -03:40:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295103_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295103_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:00.23 -00:03:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295204_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295204_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:58.64 -01:25:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295255_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295255_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:34:15.02 -05:19:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.996 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295281_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295281_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:21.41 -05:50:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.718 3100935640049817728 105.08895116582 -05.84376213725 12.7701 11.8846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 295387_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295387_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (73.2") between the two second-epoch detections
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Considering the candidate 295400_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295400_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (346.4") between the two second-epoch detections
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Considering the candidate 295414_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295414_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (208.7") between the two second-epoch detections
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Considering the candidate 295449_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295449_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (582.8") between the two second-epoch detections
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Considering the candidate 295596_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295596_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:33.76 -01:39:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295741_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 295741_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 295773_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295773_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (573.9") between the two second-epoch detections
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Considering the candidate 295783_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295783_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (326.6") between the two second-epoch detections
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Considering the candidate 295983_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 295983_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (233.0") between the two second-epoch detections
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Considering the candidate 296002_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296002_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:30.21 +00:57:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.846 3125804325323474944 100.37578011780 +00.96206277387 13.1485 12.7058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296232_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 296232_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 296248_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296248_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (492.4") between the two second-epoch detections
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Considering the candidate 296305_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296305_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:15.00 -05:59:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296374_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296374_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (61.3") between the two second-epoch detections
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Considering the candidate 296380_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296380_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:13.67 +01:34:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.498 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296567_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 296567_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 296591_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296591_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (73.5") between the two second-epoch detections
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Considering the candidate 296594_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296594_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:32:16.86 -00:38:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.520 3119243878740239232 098.06955371997 -00.63829544686 13.0812 12.2466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296669_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296669_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:03.33 -06:07:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 296683_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296683_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (106.3") between the two second-epoch detections
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Considering the candidate 296687_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 296687_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 296782_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296782_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (401.1") between the two second-epoch detections
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Considering the candidate 296797_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 296797_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 296805_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 296805_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 296975_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296975_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:31:44.91 -05:21:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.508 3103494100525069184 097.93730161631 -05.36031299715 13.1083 12.5894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 296992_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 296992_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (166.2") between the two second-epoch detections
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Considering the candidate 297080_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297080_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (232.6") between the two second-epoch detections
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Considering the candidate 297144_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297144_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:28.52 -04:07:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 297181_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297181_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 297324_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297324_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (174.0") between the two second-epoch detections
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Considering the candidate 297330_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297330_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:06.99 -01:31:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.775 3118812874479474048 098.77860290306 -01.52424273167 13.1457 12.5678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297345_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297345_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (203.9") between the two second-epoch detections
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Considering the candidate 297423_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297423_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:58:38.89 -04:20:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 4.283 3101710349067118720 104.66302468638 -04.33867408529 13.0563 12.0264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297519_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297519_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (103.0") between the two second-epoch detections
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Considering the candidate 297555_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297555_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:26.28 +02:03:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.019 3126362769851744256 101.85924991798 +02.06333923017 13.2439 12.7224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297563_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 297563_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 297565_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297565_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 297587_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 297587_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 297680_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297680_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:54.24 +00:00:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.563 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 297736_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297736_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (402.7") between the two second-epoch detections
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Considering the candidate 297769_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297769_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (143.7") between the two second-epoch detections
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Considering the candidate 297886_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 297886_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 297980_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 297980_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:26.10 -06:06:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298041_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298041_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (111.6") between the two second-epoch detections
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Considering the candidate 298049_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298049_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (153.0") between the two second-epoch detections
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Considering the candidate 298139_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298139_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:30.04 -04:07:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298320_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298320_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:52.64 -04:47:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.803 3101629122646359040 104.96985275355 -04.79110958798 13.3251 12.7714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 298359_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298359_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (533.8") between the two second-epoch detections
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Considering the candidate 298363_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298363_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (291.5") between the two second-epoch detections
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Considering the candidate 298431_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298431_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:03.92 -03:46:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298502_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298502_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:50.66 +01:35:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298512_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 298512_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 298529_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298529_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (79.0") between the two second-epoch detections
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Considering the candidate 298578_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298578_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (219.3") between the two second-epoch detections
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Considering the candidate 298582_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298582_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (96.8") between the two second-epoch detections
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Considering the candidate 298701_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 298701_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 298713_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298713_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (526.4") between the two second-epoch detections
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Considering the candidate 298879_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298879_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:25.53 -05:20:08.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 298928_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 298928_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 298938_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298938_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (109.4") between the two second-epoch detections
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Considering the candidate 298939_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 298939_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:01.70 -04:08:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298990_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 298990_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 299025_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 299025_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (260.5") between the two second-epoch detections
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Considering the candidate 299217_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 299217_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (230.8") between the two second-epoch detections
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Considering the candidate 299379_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299379_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 299422_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 299422_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:36.03 +01:59:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299470_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299470_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299476_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 299476_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (205.6") between the two second-epoch detections
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Considering the candidate 299481_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299481_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 299585_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299585_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 299843_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 299843_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:07.31 -01:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299957_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299957_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 299973_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299973_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 300003_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300003_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (123.2") between the two second-epoch detections
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Considering the candidate 300027_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300027_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:58.15 -00:53:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.820 3107328475530410368 100.49184650310 -00.89496181731 13.1913 12.1887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300057_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300057_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:14.11 -00:06:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.432 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300081_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300081_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:19.79 -03:22:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.186 3105616604643085952 100.08227451735 -03.38133788963 13.4827 13.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300116_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300116_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (39.8") between the two second-epoch detections
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Considering the candidate 300226_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300226_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (187.6") between the two second-epoch detections
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Considering the candidate 300325_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300325_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:18.56 -00:51:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.222 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300375_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 300375_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 300387_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300387_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (109.5") between the two second-epoch detections
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Considering the candidate 300537_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300537_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:12.63 -05:08:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.003 3100657291808314112 101.55197132706 -05.14813242199 13.6082 12.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300612_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300612_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (350.0") between the two second-epoch detections
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Considering the candidate 300678_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300678_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:20.64 -00:31:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.315 3113209007312878720 102.08521324729 -00.53078387966 13.4081 12.4373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300726_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300726_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:46.99 -00:16:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.489 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300908_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300908_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (109.5") between the two second-epoch detections
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Considering the candidate 300935_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300935_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (276.7") between the two second-epoch detections
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Considering the candidate 300948_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 300948_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (67.0") between the two second-epoch detections
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Considering the candidate 301079_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301079_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:25.70 -03:31:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.574 3105605746965781632 100.10561956788 -03.51895927043 13.4932 12.3498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301097_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301097_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (98.2") between the two second-epoch detections
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Considering the candidate 301135_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301135_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (151.0") between the two second-epoch detections
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Considering the candidate 301252_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301252_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:33.44 +01:51:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.870 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301417_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301417_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:59.45 -01:03:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.371 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301439_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301439_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (112.9") between the two second-epoch detections
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Considering the candidate 301465_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 301465_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 301512_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301512_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (68.6") between the two second-epoch detections
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Considering the candidate 301518_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 301518_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 301553_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301553_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (217.8") between the two second-epoch detections
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Considering the candidate 301776_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301776_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:56.60 -01:53:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.710 3106261640014320896 103.23554118099 -01.89593007242 13.7070 12.7554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301777_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301777_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 301824_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301824_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (146.6") between the two second-epoch detections
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Considering the candidate 301901_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301901_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 301903_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301903_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 301968_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301968_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 301989_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 301989_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:54.97 -02:23:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.126 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302007_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302007_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:46.53 -02:44:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.333 3106508927049985280 100.69338451398 -02.73839649824 13.7626 13.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302202_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 302202_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 302208_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302208_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:59.82 -02:44:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.976 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302214_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302214_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (216.0") between the two second-epoch detections
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Considering the candidate 302295_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 302295_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 302390_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302390_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:43.72 +01:49:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.054 3126715992262401792 099.43300290905 +01.81852126789 13.7099 12.7656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302412_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 302412_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 302453_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302453_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (86.2") between the two second-epoch detections
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Considering the candidate 302460_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302460_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:08.72 -02:34:01.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 302516_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302516_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:14.37 +00:45:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.338 3125565078465888768 101.55954576647 +00.75816110703 13.9059 12.9956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302558_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 302558_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 302579_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302579_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:40.02 -00:26:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.770 3112511367183611136 103.66730236160 -00.44919517720 13.9757 13.1957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302820_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302820_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (41.0") between the two second-epoch detections
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Considering the candidate 302900_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302900_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (69.2") between the two second-epoch detections
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Considering the candidate 302921_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302921_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:23.16 -02:46:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.398 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 302949_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 302949_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:37.02 -01:46:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.642 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67235_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 67235_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:53.25 -05:55:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:00.82 +01:46:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (303.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-04_22-19-38_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (371.4") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 102s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:47:27.93 -01:05:51.0
06:42:40.75 -00:18:15.7
06:53:52.24 -02:12:22.2
06:40:43.54 -01:24:12.5
06:57:55.40 -04:37:50.4
06:41:43.42 -01:05:57.2
06:46:17.76 -05:27:32.3
06:51:10.55 +01:05:57.1
06:48:07.19 -00:40:25.9
06:43:16.51 +00:21:47.4
06:46:13.98 +00:50:46.0
06:46:14.32 +00:51:12.0
06:49:22.87 +01:06:38.6
06:43:28.00 -03:56:25.3
06:54:34.23 -00:35:21.6
06:47:13.00 +00:51:23.8
06:51:33.02 +00:27:10.8
06:50:14.54 -00:47:14.1
06:52:07.83 +00:28:18.2
06:45:10.82 -03:57:04.3
06:51:05.17 -01:41:34.9
06:42:28.75 -06:03:12.0
06:45:04.79 -01:02:22.8
06:55:06.23 -06:05:45.5
06:44:39.55 +00:10:06.4
06:49:33.17 -01:23:30.8
06:40:17.49 -04:25:59.0
06:48:16.68 -01:48:39.5
06:45:06.27 -00:02:46.8
06:48:48.51 +00:23:29.3
06:37:44.66 -04:23:20.2
06:54:15.79 -00:38:32.5
06:47:47.49 +00:13:36.9
06:49:57.77 -05:31:46.5
06:47:11.26 -02:50:54.4
06:48:00.98 -01:06:00.2
06:46:29.61 -00:12:58.4
06:58:22.93 -04:38:16.9
06:43:46.14 +00:19:12.1
06:48:30.60 +00:57:44.2
06:49:29.21 -01:29:09.0
06:54:15.10 -02:04:21.3
06:45:33.70 -00:26:17.0
06:49:07.34 -01:40:19.1
06:51:43.99 -04:33:44.8
06:45:53.98 -00:09:38.3
06:40:18.95 -04:30:21.1
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:47:27.93 -01:05:51.0
06:42:40.75 -00:18:15.7
06:53:52.24 -02:12:22.2
06:40:43.54 -01:24:12.5
06:57:55.40 -04:37:50.4
06:41:43.42 -01:05:57.2
06:46:17.76 -05:27:32.3
06:51:10.55 +01:05:57.1
06:48:07.19 -00:40:25.9
06:43:16.51 +00:21:47.4
06:46:13.98 +00:50:46.0
06:46:14.32 +00:51:12.0
06:49:22.87 +01:06:38.6
06:43:28.00 -03:56:25.3
06:54:34.23 -00:35:21.6
06:47:13.00 +00:51:23.8
06:51:33.02 +00:27:10.8
06:50:14.54 -00:47:14.1
06:52:07.83 +00:28:18.2
06:45:10.82 -03:57:04.3
06:51:05.17 -01:41:34.9
06:42:28.75 -06:03:12.0
06:45:04.79 -01:02:22.8
06:55:06.23 -06:05:45.5
06:44:39.55 +00:10:06.4
06:49:33.17 -01:23:30.8
06:40:17.49 -04:25:59.0
06:48:16.68 -01:48:39.5
06:45:06.27 -00:02:46.8
06:48:48.51 +00:23:29.3
06:37:44.66 -04:23:20.2
06:54:15.79 -00:38:32.5
06:47:47.49 +00:13:36.9
06:49:57.77 -05:31:46.5
06:47:11.26 -02:50:54.4
06:48:00.98 -01:06:00.2
06:46:29.61 -00:12:58.4
06:58:22.93 -04:38:16.9
06:43:46.14 +00:19:12.1
06:48:30.60 +00:57:44.2
06:49:29.21 -01:29:09.0
06:54:15.10 -02:04:21.3
06:45:33.70 -00:26:17.0
06:49:07.34 -01:40:19.1
06:51:43.99 -04:33:44.8
06:45:53.98 -00:09:38.3
06:40:18.95 -04:30:21.1
###################################################################################
06:47:27.93 -01:05:51.0 -- not an asteroid (will add it to exclusion list)
06:42:40.75 -00:18:15.7 -- not an asteroid (will add it to exclusion list)
06:53:52.24 -02:12:22.2 -- not an asteroid (will add it to exclusion list)
06:40:43.54 -01:24:12.5 -- not an asteroid (will add it to exclusion list)
06:57:55.40 -04:37:50.4 -- not an asteroid (will add it to exclusion list)
06:41:43.42 -01:05:57.2 -- not an asteroid (will add it to exclusion list)
06:46:17.76 -05:27:32.3 -- not an asteroid (will add it to exclusion list)
06:51:10.55 +01:05:57.1 -- not an asteroid (will add it to exclusion list)
06:48:07.19 -00:40:25.9 -- not an asteroid (will add it to exclusion list)
06:43:16.51 +00:21:47.4 -- not an asteroid (will add it to exclusion list)
06:46:13.98 +00:50:46.0 -- not an asteroid (will add it to exclusion list)
06:46:14.32 +00:51:12.0 -- not an asteroid (will add it to exclusion list)
06:49:22.87 +01:06:38.6 -- not an asteroid (will add it to exclusion list)
06:43:28.00 -03:56:25.3 -- not an asteroid (will add it to exclusion list)
06:54:34.23 -00:35:21.6 -- not an asteroid (will add it to exclusion list)
06:47:13.00 +00:51:23.8 -- not an asteroid (will add it to exclusion list)
06:51:33.02 +00:27:10.8 -- not an asteroid (will add it to exclusion list)
06:50:14.54 -00:47:14.1 -- not an asteroid (will add it to exclusion list)
06:52:07.83 +00:28:18.2 -- not an asteroid (will add it to exclusion list)
06:45:10.82 -03:57:04.3 -- not an asteroid (will add it to exclusion list)
06:51:05.17 -01:41:34.9 -- not an asteroid (will add it to exclusion list)
06:42:28.75 -06:03:12.0 -- not an asteroid (will add it to exclusion list)
06:45:04.79 -01:02:22.8 -- not an asteroid (will add it to exclusion list)
06:55:06.23 -06:05:45.5 -- not an asteroid (will add it to exclusion list)
06:44:39.55 +00:10:06.4 -- not an asteroid (will add it to exclusion list)
06:49:33.17 -01:23:30.8 -- not an asteroid (will add it to exclusion list)
06:40:17.49 -04:25:59.0 -- not an asteroid (will add it to exclusion list)
06:48:16.68 -01:48:39.5 -- not an asteroid (will add it to exclusion list)
06:45:06.27 -00:02:46.8 -- not an asteroid (will add it to exclusion list)
06:48:48.51 +00:23:29.3 -- not an asteroid (will add it to exclusion list)
06:37:44.66 -04:23:20.2 -- not an asteroid (will add it to exclusion list)
06:54:15.79 -00:38:32.5 -- not an asteroid (will add it to exclusion list)
06:47:47.49 +00:13:36.9 -- not an asteroid (will add it to exclusion list)
06:49:57.77 -05:31:46.5 -- not an asteroid (will add it to exclusion list)
06:47:11.26 -02:50:54.4 -- not an asteroid (will add it to exclusion list)
06:48:00.98 -01:06:00.2 -- not an asteroid (will add it to exclusion list)
06:46:29.61 -00:12:58.4 -- not an asteroid (will add it to exclusion list)
06:58:22.93 -04:38:16.9 -- not an asteroid (will add it to exclusion list)
06:43:46.14 +00:19:12.1 -- not an asteroid (will add it to exclusion list)
06:48:30.60 +00:57:44.2 -- not an asteroid (will add it to exclusion list)
06:49:29.21 -01:29:09.0 -- not an asteroid (will add it to exclusion list)
06:54:15.10 -02:04:21.3 -- not an asteroid (will add it to exclusion list)
06:45:33.70 -00:26:17.0 -- not an asteroid (will add it to exclusion list)
06:49:07.34 -01:40:19.1 -- not an asteroid (will add it to exclusion list)
06:51:43.99 -04:33:44.8 -- not an asteroid (will add it to exclusion list)
06:45:53.98 -00:09:38.3 -- not an asteroid (will add it to exclusion list)
06:40:18.95 -04:30:21.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:37:44.66 -04:23:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:17.49 -04:25:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:18.95 -04:30:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:43.54 -01:24:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:43.42 -01:05:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:28.75 -06:03:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:40.75 -00:18:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:16.51 +00:21:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:28.00 -03:56:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:46.14 +00:19:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.55 +00:10:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:04.79 -01:02:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:06.27 -00:02:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:10.82 -03:57:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:33.70 -00:26:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:53.98 -00:09:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.98 +00:50:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:14.32 +00:51:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:17.76 -05:27:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:29.61 -00:12:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:11.26 -02:50:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:13.00 +00:51:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:27.93 -01:05:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:47.49 +00:13:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:00.98 -01:06:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:07.19 -00:40:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:16.68 -01:48:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:30.60 +00:57:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:48.51 +00:23:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.34 -01:40:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:22.87 +01:06:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:29.21 -01:29:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:33.17 -01:23:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:57.77 -05:31:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:14.54 -00:47:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:05.17 -01:41:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.55 +01:05:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:33.02 +00:27:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:43.99 -04:33:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:07.83 +00:28:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:52.24 -02:12:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.10 -02:04:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.79 -00:38:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.23 -00:35:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:06.23 -06:05:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.40 -04:37:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:22.93 -04:38:16.9 -- 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)
06:37:44.66 -04:23:20.2 -- not a known variable star
06:40:17.49 -04:25:59.0 -- a known variable star
06:40:18.95 -04:30:21.1 -- not a known variable star
06:40:43.54 -01:24:12.5 -- a known variable star
06:41:43.42 -01:05:57.2 -- not a known variable star
06:42:28.75 -06:03:12.0 -- a known variable star
06:42:40.75 -00:18:15.7 -- a known variable star
06:43:16.51 +00:21:47.4 -- a known variable star
06:43:28.00 -03:56:25.3 -- a known variable star
06:43:46.14 +00:19:12.1 -- a known variable star
06:44:39.55 +00:10:06.4 -- a known variable star
06:45:04.79 -01:02:22.8 -- not a known variable star
06:45:06.27 -00:02:46.8 -- not a known variable star
06:45:10.82 -03:57:04.3 -- not a known variable star
06:45:33.70 -00:26:17.0 -- a known variable star
06:45:53.98 -00:09:38.3 -- not a known variable star
06:46:13.98 +00:50:46.0 -- not a known variable star
06:46:14.32 +00:51:12.0 -- not a known variable star
06:46:17.76 -05:27:32.3 -- not a known variable star
06:46:29.61 -00:12:58.4 -- a known variable star
06:47:11.26 -02:50:54.4 -- not a known variable star
06:47:13.00 +00:51:23.8 -- not a known variable star
06:47:27.93 -01:05:51.0 -- a known variable star
06:47:47.49 +00:13:36.9 -- not a known variable star
06:48:00.98 -01:06:00.2 -- not a known variable star
06:48:07.19 -00:40:25.9 -- not a known variable star
06:48:16.68 -01:48:39.5 -- not a known variable star
06:48:30.60 +00:57:44.2 -- not a known variable star
06:48:48.51 +00:23:29.3 -- a known variable star
06:49:07.34 -01:40:19.1 -- not a known variable star
06:49:22.87 +01:06:38.6 -- a known variable star
06:49:29.21 -01:29:09.0 -- not a known variable star
06:49:33.17 -01:23:30.8 -- not a known variable star
06:49:57.77 -05:31:46.5 -- a known variable star
06:50:14.54 -00:47:14.1 -- not a known variable star
06:51:05.17 -01:41:34.9 -- a known variable star
06:51:10.55 +01:05:57.1 -- not a known variable star
06:51:33.02 +00:27:10.8 -- not a known variable star
06:51:43.99 -04:33:44.8 -- not a known variable star
06:52:07.83 +00:28:18.2 -- not a known variable star
06:53:52.24 -02:12:22.2 -- not a known variable star
06:54:15.10 -02:04:21.3 -- a known variable star
06:54:15.79 -00:38:32.5 -- not a known variable star
06:54:34.23 -00:35:21.6 -- not a known variable star
06:55:06.23 -06:05:45.5 -- not a known variable star
06:57:55.40 -04:37:50.4 -- a known variable star
06:58:22.93 -04:38:16.9 -- not a known variable star
Found 30 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
47 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 47 (excluding asteroids and hot pixels, 30 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)2461135.63815995 -observatory V36
23:16:02.70 -06:45:25.0 Mercury (0.3mag)
02:16:31.09 +13:23:02.3 Venus (-3.9mag)
23:46:53.23 -02:32:28.0 Mars (1.2mag)
07:08:20.86 +22:52:59.3 Jupiter (-2.2mag)
00:24:16.82 +00:18:10.8 Saturn (0.9mag)
03:45:31.31 +19:40:26.3 Uranus (5.8mag)
00:09:23.13 -00:24:35.3 Neptune (7.8mag)
20:33:10.17 -22:52:31.2 Pluto (14.5mag)
15:05:50.03 -22:46:48.4 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 362 Apr 4 22:23 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461135.63815995:
07:08:13.46 +22:53:14.7 Io (5.7mag)
07:08:19.31 +22:53:05.3 Europa (5.8mag)
07:08:01.63 +22:53:39.5 Ganymede (5.3mag)
07:08:01.29 +22:53:28.1 Callisto (6.5mag)
07:12:05.81 +22:46:03.0 Himalia (15.3mag)
07:08:24.83 +22:52:50.1 Thebe (16.2mag)
07:12:01.94 +23:14:34.5 Elara (17.2mag)
07:06:29.39 +23:38:40.9 Pasiphae (17.3mag)
07:16:53.85 +22:49:47.3 Carme (18.4mag)
00:24:08.64 +00:18:20.0 Titan (8.8mag)
00:24:18.87 +00:18:24.5 Rhea (10.1mag)
00:24:19.82 +00:19:51.2 Iapetus (11.5mag)
00:24:14.77 +00:18:03.2 Hyperion (14.8mag)
00:26:01.77 +00:28:06.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 4 22:23 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461135.63815995:
14:41:00.54 -07:19:03.9 JWST
20:09:19.35 -05:48:27.1 Chandra
16:49:41.52 -52:29:27.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 4 22:23 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461135.63815995 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:46:29.70 -28:10:50.7 14.0mag P/2010 H2 (Vales)
04:59:25.39 -70:12:09.9 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:24.00 +31:22:12.6 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.52 +09:14:31.7 17.6mag C/2021 G2 (ATLAS)
23:07:00.66 +28:49:59.7 17.0mag C/2022 E2 (ATLAS)
04:16:48.64 +25:44:02.9 15.9mag C/2022 N2 (PANSTARRS)
09:01:46.22 +31:53:15.5 16.1mag C/2022 QE78 (ATLAS)
08:29:55.48 -01:21:13.0 17.3mag C/2022 R6 (PANSTARRS)
18:55:43.72 +17:36:12.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:46.15 -11:40:28.2 17.6mag P/2023 B1 (PANSTARRS)
09:13:28.85 -13:40:57.7 17.5mag C/2023 F3 (ATLAS)
21:42:12.50 +62:19:08.8 17.5mag C/2023 H5 (Lemmon)
19:27:01.97 -03:35:57.4 14.3mag C/2023 R1 (PANSTARRS)
21:42:51.50 +84:28:49.4 17.8mag C/2023 X2 (Lemmon)
06:14:19.78 +63:35:40.3 17.0mag C/2024 A1 (ATLAS)
04:48:30.60 +14:04:57.8 10.3mag C/2024 E1 (Wierzchos)
16:25:39.89 +04:36:17.1 17.4mag C/2024 G6 (ATLAS)
20:17:08.12 +12:24:53.6 14.7mag C/2024 J3 (ATLAS)
03:16:52.23 -24:05:37.2 16.4mag C/2024 T5 (ATLAS)
05:07:53.44 +48:07:21.8 17.7mag C/2025 J1 (Borisov)
14:23:14.63 +36:18:28.5 14.7mag C/2025 L1 (ATLAS)
03:08:50.55 -24:35:59.8 17.7mag C/2025 Q3 (ATLAS)
22:51:01.58 +19:49:44.2 10.3mag C/2025 R3 (PANSTARRS)
12:58:50.92 +02:19:23.0 17.5mag C/2025 Y1 (ATLAS)
01:08:36.03 +05:18:18.2 3.8mag C/2026 A1 (MAPS)
23:27:35.61 +35:00:30.6 14.2mag C/2026 B2 (Sun-Gao)
18:21:43.70 -10:16:02.9 12.5mag 10P/Tempel
15:14:07.56 +04:11:39.7 13.0mag 24P/Schaumasse
11:06:07.95 -01:54:08.8 15.7mag 29P/Schwassmann-Wachmann
17:56:08.22 -10:02:09.5 17.7mag 40P/Vaisala
10:39:08.63 -05:02:50.4 16.7mag 43P/Wolf-Harrington
01:31:56.22 +15:36:43.3 17.1mag 47P/Ashbrook-Jackson
06:51:33.35 +39:17:54.6 17.1mag 63P/Wild
23:14:54.51 -12:47:14.9 15.7mag 65P/Gunn
03:35:00.82 +17:20:32.0 15.8mag 76P/West-Kohoutek-Ikemura
00:41:47.74 +06:04:29.6 14.5mag 78P/Gehrels
22:29:10.69 -12:34:34.1 14.5mag 88P/Howell
01:40:18.98 +17:38:55.9 15.1mag 93P/Lovas
04:35:05.34 +31:39:51.0 16.3mag 123P/West-Hartley
08:16:58.57 +43:22:37.8 16.2mag 124P/Mrkos
02:16:37.73 +13:08:06.9 16.4mag 128P/Shoemaker-Holt
02:26:21.46 +13:06:55.3 17.5mag 131P/Mueller
00:30:39.77 +09:11:46.2 11.3mag 141P/Machholz
00:40:42.26 +00:48:40.4 11.4mag 141P-A/Machholz
23:31:53.92 -02:44:57.7 14.2mag 141P-D/Machholz
01:09:38.94 +02:27:26.9 17.9mag 141P-I/Machholz
00:32:13.36 -06:56:09.4 15.2mag 162P/SidingSpring
10:31:20.35 +31:33:58.8 17.8mag 164P/Christensen
06:16:30.64 +24:32:48.0 17.8mag 198P/ODAS
15:10:30.02 -01:19:45.9 17.3mag 210P/Christensen
21:05:29.66 -14:04:29.7 17.4mag 218P/LINEAR
17:11:59.16 -15:11:20.9 16.2mag 235P/LINEAR
05:11:28.56 +33:45:10.2 16.6mag 240P/NEAT
07:33:48.72 -06:24:51.8 17.6mag 242P/Spahr
15:46:13.21 +06:13:56.8 17.6mag 391P/Kowalski
07:30:37.91 +21:18:09.8 17.6mag 450P/LONEOS
05:20:28.13 +45:40:28.0 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 4 22:23 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 4 22:23 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
-rw-r--r-- 1 apache apache 187K Apr 4 22:23 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:12:45.220 +03:30:21.92 AT 2026hpi 2026-03-19.82 21.35
13:05:59.910 -01:19:19.75 AT 2026hph 2026-03-19.81 22.6
11:46:36.940 +01:57:40.33 AT 2026hpg 2026-03-19.65 22.05
11:30:33.790 +02:03:55.06 AT 2026hpf 2026-03-19.65 22.36
11:29:16.830 +01:43:15.67 AT 2026hpe 2026-03-19.65 22.04
11:20:49.830 +04:08:00.92 AT 2026hpd 2026-03-19.64 22
11:03:22.060 +00:37:39.12 AT 2026hpc 2026-03-19.63 22.18
10:52:11.360 -00:09:37.37 AT 2026hpb 2026-03-19.63 22.38
10:44:39.040 +03:59:23.53 AT 2026hpa 2026-03-19.63 22.2
10:39:27.590 +02:55:53.65 AT 2026hoz 2026-03-19.63 22.5
11:13:53.930 -02:04:37.04 AT 2026hoy 2026-03-19.57 22.08
11:32:56.040 +05:15:39.22 AT 2026hox 2026-03-13.75 21.79
14:19:03.910 +04:14:08.30 AT 2026how 2026-03-09.90 22.06
13:42:38.650 +04:05:57.15 AT 2026hov 2026-03-26.90 22.47
10:27:51.570 +00:48:59.98 AT 2026hou 2026-03-22.63 22.25
13:58:28.600 +02:11:38.08 AT 2026hot 2026-03-19.83 22.42
07:15:34.880 +25:58:24.77 AT 2026hos 2026-03-20.27 20.6179
06:14:25.910 +51:19:28.34 AT 2026hor 2026-03-25.14 20.2907
19:09:43.670 +04:40:04.90 AT 2026hoq 2026-03-25.91 16.32
13:14:45.263 +13:33:04.46 AT 2026hop 2026-03-28.45 19.632
-rw-r--r-- 1 apache apache 29K Apr 4 22:23 tns_transients_list.txt
