This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AG Mon,2461140.6741,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AG Mon 20260410.1741 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105498952598830592,2461140.6741,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105498952598830592 20260410.1741 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8483-01.1646,2461140.6741,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8483-01.1646 20260410.1741 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102745917223873536,2461140.6741,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102745917223873536 20260410.1741 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8293-02.8820,2461140.6741,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8293-02.8820 20260410.1741 13.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1270+01.8462,2461140.6741,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1270+01.8462 20260410.1741 13.68CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3944-03.6481,2461140.6741,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3944-03.6481 20260410.1741 13.64CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.34CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1718-00.9990,2461140.6741,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1718-00.9990 20260410.1741 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2029+02.1494,2461140.6741,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2029+02.1494 20260410.1741 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109773617594128256,2461140.6741,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109773617594128256 20260410.1741 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2607+01.7289,2461140.6741,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2607+01.7289 20260410.1741 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112091422462107520,2461140.6741,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112091422462107520 20260410.1741 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4280-01.9828,2461140.6741,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4280-01.9828 20260410.1741 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102314182812686976,2461140.6741,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102314182812686976 20260410.1741 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0207+00.9747,2461140.6741,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0207+00.9747 20260410.1741 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.4965-00.6001,2461140.6741,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.4965-00.6001 20260410.1741 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113790030488561920,2461140.6741,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113790030488561920 20260410.1741 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2328-03.1983,2461140.6741,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2328-03.1983 20260410.1741 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109907586213358720,2461140.6741,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109907586213358720 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113254808845036928,2461140.6741,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113254808845036928 20260410.1741 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9165-01.7520,2461140.6741,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9165-01.7520 20260410.1741 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110797950110765952,2461140.6741,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110797950110765952 20260410.1741 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0351+01.0281,2461140.6741,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0351+01.0281 20260410.1741 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.21CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101577514319516416,2461140.6741,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101577514319516416 20260410.1741 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111162743151960064,2461140.6741,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111162743151960064 20260410.1741 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3135936153174376576,2461140.6741,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3135936153174376576 20260410.1741 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059186977386269312,2461140.6741,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059186977386269312 20260410.1741 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126029961425668224,2461140.6741,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126029961425668224 20260410.1741 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114778491440223488,2461140.6741,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114778491440223488 20260410.1741 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6002-04.1912,2461140.6741,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6002-04.1912 20260410.1741 12.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114737878230131072,2461140.6741,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114737878230131072 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107739143129547392,2461140.6741,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107739143129547392 20260410.1741 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114369370035090176,2461140.6741,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114369370035090176 20260410.1741 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114569137555198464,2461140.6741,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114569137555198464 20260410.1741 12.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109841924755441024,2461140.6741,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109841924755441024 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6438-00.3074,2461140.6741,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6438-00.3074 20260410.1741 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.9050-02.3273,2461140.6741,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.9050-02.3273 20260410.1741 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4191-04.3825,2461140.6741,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4191-04.3825 20260410.1741 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107388433273617792,2461140.6741,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107388433273617792 20260410.1741 12.86CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.5480-02.0407,2461140.6741,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.5480-02.0407 20260410.1741 12.86CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.3925-03.5224,2461140.6741,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.3925-03.5224 20260410.1741 12.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6699+01.3042,2461140.6741,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.6699+01.3042 20260410.1741 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0154-01.7229,2461140.6741,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0154-01.7229 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053011084987857408,2461140.6741,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053011084987857408 20260410.1741 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7707-03.1723,2461140.6741,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7707-03.1723 20260410.1741 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119584113167330944,2461140.6741,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119584113167330944 20260410.1741 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.6372-00.9527,2461140.6741,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.6372-00.9527 20260410.1741 12.61CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0115-03.3931,2461140.6741,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0115-03.3931 20260410.1741 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107274358943072000,2461140.6741,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107274358943072000 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.5157-01.0853,2461140.6741,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.5157-01.0853 20260410.1741 12.61CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109500251512786944,2461140.6741,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109500251512786944 20260410.1741 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059503361857653632,2461140.6741,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059503361857653632 20260410.1741 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.7201-00.0697,2461140.6741,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.7201-00.0697 20260410.1741 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101673034391323264,2461140.6741,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101673034391323264 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112897600704147072,2461140.6741,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112897600704147072 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.2532-02.1619,2461140.6741,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.2532-02.1619 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.8710+01.9494,2461140.6741,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8710+01.9494 20260410.1741 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064143.42-010627.5,2461140.6741,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064143.42-010627.5 20260410.1741 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059266687674749696,2461140.6741,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059266687674749696 20260410.1741 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.7416-04.3083,2461140.6741,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.7416-04.3083 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107032775621691520,2461140.6741,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107032775621691520 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.3712-04.1472,2461140.6741,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.3712-04.1472 20260410.1741 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105979580920754432,2461140.6741,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105979580920754432 20260410.1741 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108383555718321408,2461140.6741,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108383555718321408 20260410.1741 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115211321064418944,2461140.6741,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115211321064418944 20260410.1741 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.2601+02.8485,2461140.6741,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.2601+02.8485 20260410.1741 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059224670018297728,2461140.6741,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059224670018297728 20260410.1741 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1090+01.9830,2461140.6741,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.1090+01.9830 20260410.1741 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0640542+000137,2461140.6741,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0640542+000137 20260410.1741 11.64CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101821880779349888,2461140.6741,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101821880779349888 20260410.1741 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109303606430140928,2461140.6741,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109303606430140928 20260410.1741 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112276892032630400,2461140.6741,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112276892032630400 20260410.1741 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108445441905316864,2461140.6741,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108445441905316864 20260410.1741 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114604936102169856,2461140.6741,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114604936102169856 20260410.1741 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109822923819222400,2461140.6741,9.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109822923819222400 20260410.1741 9.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119852462723061120,2461140.6741,9.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119852462723061120 20260410.1741 9.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.0773+01.7811,2461140.6741,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.0773+01.7811 20260410.1741 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9174+00.4331,2461140.6741,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9174+00.4331 20260410.1741 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1631+01.7787,2461140.6741,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1631+01.7787 20260410.1741 11.26CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127192493115969152,2461140.6741,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127192493115969152 20260410.1741 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CD Mon,2461140.6741,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CD Mon 20260410.1741 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111447039926977152,2461140.6741,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111447039926977152 20260410.1741 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110157583366513664,2461140.6741,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110157583366513664 20260410.1741 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119213405948991232,2461140.6741,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119213405948991232 20260410.1741 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119280785395344512,2461140.6741,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119280785395344512 20260410.1741 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059182270101246208,2461140.6741,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059182270101246208 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059651314888833408,2461140.6741,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059651314888833408 20260410.1741 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112749274012032640,2461140.6741,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112749274012032640 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J110.5120+00.7391,2461140.6741,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J110.5120+00.7391 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111409553452325120,2461140.6741,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111409553452325120 20260410.1741 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059210719964348544,2461140.6741,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059210719964348544 20260410.1741 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111644058665914496,2461140.6741,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111644058665914496 20260410.1741 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0707331-032533,2461140.6741,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0707331-032533 20260410.1741 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105621277567743360,2461140.6741,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105621277567743360 20260410.1741 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107474882374152960,2461140.6741,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107474882374152960 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J109.0122+02.1631,2461140.6741,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J109.0122+02.1631 20260410.1741 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2174-00.5958,2461140.6741,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2174-00.5958 20260410.1741 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127764887696264704,2461140.6741,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127764887696264704 20260410.1741 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115633327372214656,2461140.6741,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115633327372214656 20260410.1741 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3110006336102386176,2461140.6741,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3110006336102386176 20260410.1741 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.6061-07.0282,2461140.6741,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6061-07.0282 20260410.1741 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114520003127512192,2461140.6741,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114520003127512192 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127198604847054208,2461140.6741,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127198604847054208 20260410.1741 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107955953073281024,2461140.6741,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107955953073281024 20260410.1741 12.61CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.5386+00.9385,2461140.6741,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.5386+00.9385 20260410.1741 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3331+02.7602,2461140.6741,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.3331+02.7602 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070449.39+023047.8,2461140.6741,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J070449.39+023047.8 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461140.6741,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0676-03.0161 20260410.1741 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120812576892617856,2461140.6741,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120812576892617856 20260410.1741 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.6148+02.3383,2461140.6741,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.6148+02.3383 20260410.1741 12.86CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2998-03.9607,2461140.6741,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2998-03.9607 20260410.1741 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111108768303524224,2461140.6741,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111108768303524224 20260410.1741 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126395106665966080,2461140.6741,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126395106665966080 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7477+00.2283,2461140.6741,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7477+00.2283 20260410.1741 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100783735647123712,2461140.6741,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100783735647123712 20260410.1741 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107712170734171776,2461140.6741,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107712170734171776 20260410.1741 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105133506722636672,2461140.6741,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105133506722636672 20260410.1741 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126271617766100608,2461140.6741,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126271617766100608 20260410.1741 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127217163407760640,2461140.6741,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127217163407760640 20260410.1741 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.6757+01.6632,2461140.6741,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6757+01.6632 20260410.1741 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120480691881910656,2461140.6741,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120480691881910656 20260410.1741 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126153111029053568,2461140.6741,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126153111029053568 20260410.1741 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101029201615746048,2461140.6741,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101029201615746048 20260410.1741 12.86CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3104844811903742208,2461140.6741,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3104844811903742208 20260410.1741 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126952627779842688,2461140.6741,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126952627779842688 20260410.1741 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113913996125565440,2461140.6741,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260410.1741 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3127840174182358016,2461140.6741,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3127840174182358016 20260410.1741 12.91CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.6630+01.9547,2461140.6741,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.6630+01.9547 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17100,2461140.6741,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 17100 20260410.1741 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.4835+00.2927,2461140.6741,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.4835+00.2927 20260410.1741 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108875037416696192,2461140.6741,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108875037416696192 20260410.1741 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108661461582071936,2461140.6741,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108661461582071936 20260410.1741 13.21CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461140.6741,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9913-01.3476 20260410.1741 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.0276-01.3052,2461140.6741,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0276-01.3052 20260410.1741 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105320458058531328,2461140.6741,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105320458058531328 20260410.1741 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108081194321500032,2461140.6741,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108081194321500032 20260410.1741 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113525082544566656,2461140.6741,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113525082544566656 20260410.1741 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106320906260060800,2461140.6741,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106320906260060800 20260410.1741 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J063831.30+022536.6,2461140.6741,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063831.30+022536.6 20260410.1741 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100477590376004224,2461140.6741,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100477590376004224 20260410.1741 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J108.1277+01.2122,2461140.6741,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.1277+01.2122 20260410.1741 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112636294895145472,2461140.6741,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112636294895145472 20260410.1741 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.8055-05.8431,2461140.6741,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8055-05.8431 20260410.1741 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.9421-02.1958,2461140.6741,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9421-02.1958 20260410.1741 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106045203719510272,2461140.6741,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106045203719510272 20260410.1741 13.27CV 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 10.1741 2461140.6741 13.19 06:38:53.45 -00:49:17.5
212.23250 -3.16621 galactic Mon Second-epoch detections are separated by 2.6" and 7.9 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 3119330469578499072 | 06:38:54.14 -00:50:00.1 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A0 1949AnHar.112....1C HD 291993 J-Ks=0.366+/-0.043 (G)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3119330469578499072,2461140.6741,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3119330469578499072 20260410.1741 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111710166803566464,2461140.6741,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111710166803566464 20260410.1741 13.21CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125817485103519104,2461140.6741,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125817485103519104 20260410.1741 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3120615729951778688,2461140.6741,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3120615729951778688 20260410.1741 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6741,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1741 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107455911497806848,2461140.6741,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107455911497806848 20260410.1741 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114123113791163520,2461140.6741,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114123113791163520 20260410.1741 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115387616581722368,2461140.6741,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115387616581722368 20260410.1741 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102574299,2461140.6741,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102574299 20260410.1741 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8095-01.6362,2461140.6741,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8095-01.6362 20260410.1741 13.50CV 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
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BM Mon,2461140.6741,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BM Mon 20260410.1741 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RR Mon,2461140.6741,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RR Mon 20260410.1741 10.94CV 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
Date (UTC)
JD(UTC)
mag.
R.A. & Dec.(J2000)
X & Y (pix)
Image
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AI Mon,2461140.6741,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AI Mon 20260410.1741 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
## 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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461140.67453978 10.04.2026 04:11:10.237 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
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: 8 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): 34684
Objects passed selection criteria: 34620
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 29950.5
Average stars matched: 29064.8 (97.0426 %)
Memory usage VmPeak: 136944 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 23:24:10 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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461140.67453978 10.04.2026 04:11:10.237 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 530
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 209 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): 243912
Objects passed selection criteria: 243387
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 220350
Average stars matched: 212234 (96.3168 %)
Memory usage VmPeak: 1994976 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 23:30:34 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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: 2461140.67372288
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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits'
wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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 06:51:31.627 -02:00:27.93
Angular distance between the image centers 0.0478 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 06:51:29.337 -01:59:59.67
Angular distance between the image centers 0.0574 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 06:51:31.627 -02:00:27.93
Second-epoch second image center 06:51:29.337 -01:59:59.67
Angular distance between the image centers 0.01235 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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.aTfr3NejQa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.4ToxayQR7r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits &> /tmp/tmp.leYQm5MlL0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits &> /tmp/tmp.buBnZXBqDz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_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 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
2.3 pix fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.5 mag. fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
14.5 mag. fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (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.aTfr3NejQa (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
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...
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
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"
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.4ToxayQR7r (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
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.leYQm5MlL0 (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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2430, passed=23876
Got 23876 stars (including 21412 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat
util/solve_plate_with_UCAC5 got 23876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 23075 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 23074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 23074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 931 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.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.buBnZXBqDz (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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2433, passed=23656
Got 23656 stars (including 21205 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat
util/solve_plate_with_UCAC5 got 23656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 22983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 22986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 22986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52790.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52507_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 52507_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:44.60 -03:25:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.461 3108049686441841152 108.43592082976 -03.42017790830 12.1599 11.7721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 52511_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 52511_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:36:11.59 -04:05:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 1.549 3104814132953812608 099.04809791000 -04.09569004411 11.5936 10.8079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52512_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 52512_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:16:02.26 -02:48:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52513_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 52513_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:38:08.54 -01:28:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.518 3106909218001458560 099.53605034664 -01.47152094130 11.0094 10.4057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52516_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 52516_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:22:36.64 +01:09:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52651_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 52651_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:06.38 +01:45:32.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52790_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 52790_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53386_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 53386_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:08.92 -04:00:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.536 3059701273947972352 110.03724138987 -04.01122578037 12.1004 11.8965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53418_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 53418_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:59:25.56 +02:56:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 4.367 3115879716757328640 104.85575435950 +02.93609786286 12.1168 11.1870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 01285_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:53.12 -06:53:22.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.69 -02:21:30.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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 06:51:31.627 -02:00:27.93
Angular distance between the image centers 0.0478 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 06:51:29.337 -01:59:59.67
Angular distance between the image centers 0.0574 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 06:51:31.627 -02:00:27.93
Second-epoch second image center 06:51:29.337 -01:59:59.67
Angular distance between the image centers 0.01235 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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.xITjzo5Vpw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.ig1JVqB4Ze
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits &> /tmp/tmp.Xf7KPkBDkP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits &> /tmp/tmp.lLHCF9IKcK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_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.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 500 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.8 mag. fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
13.8 mag. fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.xITjzo5Vpw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
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...
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
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"
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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_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-Q1b1x1_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.ig1JVqB4Ze (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_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-Q1b1x1_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...
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.Xf7KPkBDkP (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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=65, blended=25828, passed=185925
Got 185925 stars (including 159843 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat
util/solve_plate_with_UCAC5 got 185925 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.7)
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...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 182520 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 182521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 182519 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.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.lLHCF9IKcK (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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=64, blended=26282, passed=187452
Got 187452 stars (including 160926 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat
util/solve_plate_with_UCAC5 got 187452 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 183305 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 183311 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 183309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits -region wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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-Q1b1x1_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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q1b1x1_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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-09-59_20.00sec_-4.90C_LIGHTs_0026.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.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_2026-04-09_CI_Mon-02-Q1b1x1_231205_TTUQ1b1x1_20823_HjODFfgx/wcs_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out228912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290517.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out291952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out292999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293569.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out294425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out294436.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out294985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out288374.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out199360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out270041.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out288344.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out288375.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out288386.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out289057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291360.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292144.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out292995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294958.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 241s
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: 127s
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Considering the candidate 288168_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288168_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:39:39.09 +01:46:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.230 3126682457158053888 099.91295478118 +01.77544117855 14.1799 13.1673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288172_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288172_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:56:53.40 -01:17:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288180_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288180_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:45.85 -02:37:44.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 288181_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288181_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288183_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288183_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288189_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288189_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:58.46 -02:48:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.685 3108008111155593472 106.49343500289 -02.81698093305 14.4799 13.8964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288190_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288190_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:33.64 -00:20:43.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288193_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288193_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288199_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288199_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288200_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288200_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288201_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288201_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:18.86 +01:14:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.359 3114662458604743168 106.82828975608 +01.24703090987 14.3765 13.9492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288210_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288210_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:28.33 +03:01:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.718 3127842063967195392 103.61773770839 +03.02715183520 14.0948 13.0576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288214_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288214_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:42:41.61 -03:32:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.778 3105572418019801216 100.67337610879 -03.54957724967 14.2149 13.4973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288220_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288220_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:57:58.87 -03:42:37.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288226_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288226_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288227_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288227_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288233_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288233_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288245_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288245_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:53:45.79 +01:43:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.627 3114190768115468544 103.44074071667 +01.72916096446 14.2925 13.7012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288260_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288260_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:45:11.73 +00:14:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.888 3125505739198071040 101.29884931989 +00.24208721242 14.2269 13.7415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288264_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288264_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288271_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288271_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288272_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288272_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:51:40.90 -00:36:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.727 3113168737700080512 102.92004431007 -00.61391037011 14.4502 13.8851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288275_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288275_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:58:53.76 +01:27:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.253 3113930694955439360 104.72333172725 +01.44873045792 14.1228 13.8043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288278_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288278_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:47:23.72 +01:30:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.542 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288281_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288281_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288287_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288287_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288292_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288292_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:54.53 +02:17:58.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288294_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288305_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288305_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288311_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288311_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288320_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288320_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288321_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288321_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288323_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288323_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 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 288324_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288324_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:53.77 +02:24:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.774 3115787362079041408 105.47381410161 +02.41558772913 14.0703 13.5780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288325_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288325_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288332_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288332_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:49:53.31 +01:01:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.030 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288333_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288333_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:19.85 -00:56:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.785 3112568954105823744 105.33361949851 -00.94546764897 14.2680 13.7804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288334_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288334_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:10:58.26 +01:34:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.858 3114502548380715520 107.74239617038 +01.57955882098 14.3309 13.6880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288337_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288337_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288341_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288341_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288344_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288344_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288350_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288350_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 288353_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288353_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288354_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288354_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:26.31 +00:51:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.712 3111540704573294592 109.85936267711 +00.85671446621 13.9242 13.3488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288356_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288356_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288359_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288359_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288366_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288366_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:08:17.16 -04:56:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.817 3059427667355169920 107.07112402067 -04.93442171047 14.0267 13.6990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288367_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288368_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288368_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:05.41 +02:16:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288369_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288369_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:19.14 +00:32:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.799 3111506035597560064 109.57968980214 +00.54547492736 13.8524 12.8928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288374_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288374_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:08:47.42 -00:37:50.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 288375_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288375_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288377_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288379_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288379_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:20.78 +02:39:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288386_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288386_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288393_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288393_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:06:35.71 -03:35:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.279 3107814253511857152 106.64878677894 -03.59396627835 13.8153 13.0278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288397_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288397_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:16:18.34 -02:35:04.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)
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Considering the candidate 288400_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288400_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288402_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288402_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:59:51.02 -05:12:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.511 3101581706207521280 104.96246888320 -05.20313260263 13.9922 13.4966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288407_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288407_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:24.92 +01:22:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.164 3111774178995883520 109.35416649846 +01.37578121688 13.8902 13.2274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288410_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288410_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:15:24.25 -03:45:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288413_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288413_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288414_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288414_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:47:02.69 -03:47:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288417_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288417_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:12.94 -03:22:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288419_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288419_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288420_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288420_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:18.99 -01:02:03.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 288427_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288427_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288429_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288429_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288432_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288432_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:58:21.97 +02:56:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.132 3127795678321354752 104.59130772371 +02.93545583723 13.8170 12.7648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288433_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288433_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288435_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288435_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:14.31 +01:10:20.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 288437_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288437_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288440_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288440_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:44:18.28 +00:55:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.994 3125627991146452096 101.07661447301 +00.92193816340 14.0466 13.4484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288441_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288441_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:57:00.54 +01:49:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288443_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288443_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288448_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288448_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288449_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288449_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:11.32 +02:16:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.726 3126199354937805952 102.54733339303 +02.27372853445 14.0069 13.5672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288451_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288451_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:58:10.11 -00:41:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.305 3112454703675202432 104.54210947940 -00.68736231469 13.9840 13.5340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288452_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288452_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288463_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288463_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 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 288468_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288468_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288469_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288469_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288475_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288475_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288476_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288476_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288478_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288478_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:34:10.48 +02:41:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.169 3130015832814211072 098.54363334231 +02.68403698486 13.6790 13.2031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288480_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288480_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288481_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288481_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:37:56.03 +00:48:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288482_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288482_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:04.05 -00:19:28.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
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Considering the candidate 288486_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288486_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288490_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288490_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288492_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288492_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:30:15.33 +02:15:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288494_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288494_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:39:09.50 +00:12:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.089 3119735669675792640 099.78961426519 +00.20583681379 13.7793 13.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288495_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288495_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:27.72 -01:00:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.214 3109568623093291648 106.36453423089 -01.00305075955 13.7684 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288500_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288500_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:41.55 +01:46:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288502_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288502_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:41.10 -03:34:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288504_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288505_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288505_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:12.64 -02:43:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.393 3105723944466034304 101.55241972973 -02.73053379851 13.4267 12.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288506_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288506_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288510_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288510_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288511_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288511_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:12.64 -01:58:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288518_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288518_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288519_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288519_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288520_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288520_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288523_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288523_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:00:06.85 +02:57:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.526 3115877826971729792 105.02857894626 +02.96449349911 13.9092 13.3678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288524_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288524_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:42:56.91 +00:43:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.258 3125594799639377024 100.73738555000 +00.73187374331 13.4606 12.4772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288530_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288530_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:37.27 -03:19:40.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288532_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288532_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:06:51.30 -05:24:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.035 3053380834439456512 106.71297928258 -05.41131714573 13.7657 12.8790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288533_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288533_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:33.26 -02:20:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288534_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288534_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288540_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288540_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288547_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288547_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:15:07.59 -03:19:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288549_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288549_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:52.49 -06:34:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288552_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288552_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288553_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288553_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288556_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288556_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:19.33 -01:29:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.224 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288558_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288558_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288564_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288564_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:15:07.94 +02:31:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288565_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288565_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288566_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288566_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:11.60 -02:02:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288570_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288570_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288577_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288577_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:24.47 +00:13:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288579_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288579_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:34.66 +01:34:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.666 3114874007212799872 107.89391146696 +01.58006011879 13.6108 13.0873 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288580_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288584_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288584_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:51.99 -01:20:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288592_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288592_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:03.47 +02:41:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.636 3126321267588102784 103.51434648393 +02.68277649168 13.4934 12.5762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288594_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288594_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:22:43.60 -00:18:13.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:59.59 -04:42:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288599_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288599_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288601_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288601_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288602_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288602_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:45.66 -05:25:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288603_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288603_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:52.89 -01:58:40.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288609_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288609_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:42:02.19 +03:04:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.146 3127470016721948672 100.50926061391 +03.07716935730 13.5539 13.1235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288610_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288610_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:22:10.49 +00:08:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288614_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288614_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:59.76 +01:25:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.954 3114505228441453568 107.49856296580 +01.42885351832 13.7133 13.1674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288615_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288615_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:08.09 -03:40:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288616_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288616_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:50.51 +00:09:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288618_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288618_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288619_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288619_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:04:13.82 -03:33:00.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288621_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288621_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:11.56 -00:21:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288625_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288625_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288626_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288626_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:22:41.81 +02:15:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288628_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288628_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288632_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288632_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:29:29.67 -00:06:35.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288633_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288633_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288635_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288635_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:04.49 +01:03:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.201 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288636_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288636_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:59:49.41 +02:13:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.535 3115664010613672832 104.95592961789 +02.21918834243 13.2142 12.3137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288638_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288638_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288642_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288643_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288643_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:44:48.81 +03:11:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288644_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288644_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288647_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288647_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:25.46 +02:12:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 2.296 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288648_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288648_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288649_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288649_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288651_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288651_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:00.12 -00:49:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.522 3109435547827940992 107.75085395925 -00.81846770141 12.3859 11.1035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288652_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288652_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288655_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288655_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:44:18.31 -05:27:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288656_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288656_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:53.61 +02:27:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288662_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288662_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:16:32.52 -01:58:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288663_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288663_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:48:56.69 -00:22:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.062 3113217970902547328 102.23619776126 -00.37746174804 13.1252 12.0554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288665_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288665_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288666_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288666_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:41.97 -01:47:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288667_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288667_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:03.52 +01:06:36.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288672_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288675_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288675_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288678_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288678_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288681_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288681_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:30.11 -05:37:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288682_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288682_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:56:43.53 +02:46:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.417 3127766919219874688 104.18143344956 +02.78191443907 13.3299 12.8376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288683_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288683_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:41.51 -00:55:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.974 3109438369624194176 107.42284395727 -00.91850858261 13.2975 12.8620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288684_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288684_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:04:35.19 +02:44:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.243 3115638962369103616 106.14639238151 +02.74839410305 13.5299 12.7548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288687_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288687_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:08:26.28 +02:46:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.359 3115944175624624768 107.10939963129 +02.76846114600 13.3302 12.8585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288690_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288690_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288691_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288691_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288694_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288694_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288697_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288697_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288700_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288700_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288701_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288701_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:04.09 +00:11:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.899 3113368711376822016 103.51696124537 +00.19533758674 13.1448 12.3192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288703_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288703_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288707_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288707_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:21.71 +02:15:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.064 3115503000884520448 105.34023424991 +02.26334555588 13.2081 12.8723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288709_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288709_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288713_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288716_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288716_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:26.99 -05:01:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288718_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288718_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:08:42.73 +01:59:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.233 3114730692744947456 107.17833101923 +01.99528879820 13.2190 12.4774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288720_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288720_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:53:54.53 +01:48:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288723_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288723_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:42.14 -02:01:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.953 3108458739123377024 107.42547995682 -02.02695274042 13.3539 12.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288724_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288724_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:43.56 -02:48:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288725_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288725_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288729_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288729_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:42:09.72 -03:38:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.474 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288730_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288730_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:36.11 -05:28:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288731_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288731_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288732_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288732_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:44.57 -01:10:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.314 3109407033543026944 106.93571220891 -01.18078163253 12.8093 12.0987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288734_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288734_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:55.35 -05:50:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 1.903 3101120976475849088 103.23063780077 -05.83547284251 12.9729 12.5279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288736_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288736_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288741_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288741_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:36.87 +02:52:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288742_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288742_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288743_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288743_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288744_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288744_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:41:45.16 -01:18:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288746_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288746_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:04.16 -05:27:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288747_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288747_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288748_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288748_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:10:41.24 -05:05:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.411 3059365235708755072 107.67152770225 -05.08526328657 13.1344 12.9404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288749_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288752_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288752_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 288757_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288757_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:16:00.02 +01:17:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288758_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288758_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:58.67 -02:58:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.111 3107963993251302912 106.99440881430 -02.97752881737 12.9544 12.4417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288759_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288759_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:09.17 +00:52:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288761_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288761_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:16:32.80 -02:31:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288763_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288763_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:17.23 -01:27:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288764_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288764_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:26.17 +01:50:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288765_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288765_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:33.37 -02:10:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288766_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288766_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:42.92 +01:11:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.997 3111565099987318016 109.67918781625 +01.18643427167 11.0195 9.6013 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288772_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288772_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:02.39 -01:55:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 2.051 3109811997422651392 109.25974482713 -01.92788937551 12.8310 12.5097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288774_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288774_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:08.15 -05:53:00.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 288777_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288777_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:09.30 +00:34:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.372 3113585005929929984 103.03834255055 +00.57848204790 12.7509 11.9519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288778_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288778_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288780_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288780_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:33.78 -04:55:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.635 3058862037338641920 110.14055403700 -04.92537223247 12.7487 12.4557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288783_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288783_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:18.41 -01:42:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 2.422 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288785_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288785_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:56:13.93 -05:00:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.682 3101283768615588864 104.05791933885 -05.00731223009 12.7491 12.5524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288786_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288786_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:15.22 -02:52:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288788_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288788_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288790_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288790_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:45.03 -06:16:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.089 3052293451796003584 108.43763284587 -06.27583015704 12.5608 12.1000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288791_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288791_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:27.88 -03:56:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.859 3105336843354946560 100.86630214109 -03.94202624916 12.6631 12.4058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 288792_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288792_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288795_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288795_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288797_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288797_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288798_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288798_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:31:31.93 +01:02:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.902 3120742414307317632 097.88316696000 +01.04315327108 12.7165 12.2164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288801_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288801_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:53:50.72 +01:53:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288802_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288802_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288804_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288804_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288806_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288806_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:40.32 +01:01:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288808_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288808_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 288810_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288810_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:21:56.63 +01:06:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288811_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288811_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:17.72 +01:47:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288812_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288812_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:14.38 -02:12:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288813_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288813_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:50.97 -00:49:18.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288814_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288817_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288817_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:24.78 -01:42:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.057 3109118373080196224 105.35380665429 -01.71484121383 12.1150 11.6916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288820_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288820_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288822_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288822_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:52.33 -01:57:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288823_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288823_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:24.37 +01:15:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288824_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288824_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288825_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288825_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:45:59.05 -04:51:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288829_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288829_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:52.49 +00:16:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)GAIADR2_OUTPUT=# 1.282 3111435834352490752 109.96898542965 +00.27883173656 11.4762 10.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288830_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 288830_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288831_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 288831_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:33:37.77 +01:56:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289056_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 289056_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:20:21.13 -06:07:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.77, MAG_FAINT_SEARCH_LIMIT=10.75)GAIADR2_OUTPUT=# 1.182 3008152384963645184 095.08797473371 -06.12654381191 10.5149 10.2963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289057_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 289057_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289442_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 289442_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:49.50 -05:43:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289513_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 289513_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289527_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 289527_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:38.87 -03:56:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289616_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 289616_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289686_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 289686_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:37.69 +00:43:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 1.574 3119794424826044928 100.15717896773 +00.71691830212 11.9547 11.2893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289799_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 289799_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:12.94 +02:40:12.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289855_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 289855_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289878_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 289878_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:18.64 +00:20:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289965_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 289965_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290014_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290014_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:11.44 -02:19:21.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290098_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 290098_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290141_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290141_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:41.56 -00:33:41.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290209_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290209_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:29:09.46 -05:33:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290228_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290228_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:21:53.70 +02:20:44.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290243_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290243_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:38:47.86 +00:39:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 2.113 3119814529571933824 099.69953942625 +00.66545390352 11.2963 9.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290250_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290250_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:28.37 -00:24:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290296_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290296_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:58.83 +02:49:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 4.942 3116003450473542784 106.49468568923 +02.82917133305 12.4156 11.5579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290348_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290348_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:36:41.08 -05:13:20.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290406_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290406_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:00.32 -01:49:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290419_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290419_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:21:54.64 +02:22:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290517_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290517_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:47:15.77 +02:25:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 3.069 3126425545095312128 101.81640110765 +02.41641919175 12.5279 11.6391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:41.21 +00:46:12.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290664_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290664_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:22:45.41 -02:10:06.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290675_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290675_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:41:37.36 +03:12:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.351 3127486917412984320 100.40610817052 +03.20929581198 12.4224 11.5651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290688_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290688_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:11.69 -01:59:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290690_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290690_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:08.94 +00:16:35.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290746_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 290746_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290748_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290748_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:23:43.00 +02:39:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290759_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290759_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:21.58 -04:07:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 0.873 3101775525191969408 105.83967354142 -04.12738694134 12.8115 11.9175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 290766_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290766_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:18.10 +02:01:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290833_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290833_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:23.69 +00:54:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290847_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290847_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:39.58 -04:37:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 2.656 3101534633371804672 105.66529147356 -04.63116397367 12.8393 12.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290898_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290898_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:35:16.27 -04:45:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.139 3103909715920100864 098.81776045801 -04.76603712068 12.8544 12.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290905_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290905_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:38.43 +01:13:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290923_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 290923_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:21:17.06 -00:11:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.564 3121734483032022144 095.32070803228 -00.20016618751 12.9368 12.0752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290952_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 290952_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290971_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 290971_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291009_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291009_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:06:42.29 -03:09:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.596 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291010_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291010_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:26:19.58 +01:23:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.922 3123455008273752704 096.58153352703 +01.38735719100 12.8884 12.3897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291067_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291067_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:01.55 +01:48:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.210 3114755436055724928 106.25598204354 +01.81022333530 13.0723 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291163_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291163_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:30.03 -04:07:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.475 3102509449203351296 103.62527411825 -04.12544889351 12.9516 12.4533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291176_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291176_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:45:04.77 -01:02:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291244_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291244_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:22:49.94 -05:23:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291265_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291265_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:44.60 -02:33:55.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291290_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291290_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:15:55.52 -06:13:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291302_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291302_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:34:14.95 -05:19:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291331_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291331_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:26:20.81 -03:09:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.921 3117129075501324160 096.58656414943 -03.16615954689 13.2570 12.7303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291333_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291333_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:31:44.93 -05:21:33.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291360_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291360_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291371_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291371_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291379_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291379_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:13.54 +01:34:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.823 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291414_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291414_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:32:16.69 -00:38:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291427_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291427_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:18.95 +02:16:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.839 3126841542746665088 100.07927776885 +02.27567706898 13.2041 12.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291432_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291432_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:29:22.97 +02:43:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291445_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291445_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:44:07.32 +03:13:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 3.945 3127311648388618880 101.03050410819 +03.21757088990 13.2680 12.7484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291446_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291446_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291457_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291457_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:17.48 -04:25:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291470_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291470_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291523_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291523_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291547_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291547_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291589_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291589_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291593_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291593_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291594_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291594_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:52.25 +01:55:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291636_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291636_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:59.11 -01:54:01.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291638_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291638_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:56:45.68 +00:46:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.261 3113784979607011712 104.19017946265 +00.76807653068 13.3516 13.0131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291645_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291645_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291652_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291652_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:03.31 -02:29:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.887 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291700_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291700_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:10.61 -00:58:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291725_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291725_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:48.15 -04:14:28.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291744_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291744_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:01.57 -02:44:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291806_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291806_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:25:20.42 +02:55:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291829_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291829_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291834_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291834_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:44:11.59 +03:13:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.997 3127311480888772096 101.04831658328 +03.21883456912 13.4524 12.9837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 291844_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291844_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:23:57.56 -04:42:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291845_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291845_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291848_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291848_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:26:04.91 -04:38:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291868_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291868_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:47.28 -04:14:50.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 291874_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291874_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291907_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291907_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:55.09 -02:23:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291915_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291915_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291925_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291925_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291952_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 291952_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:22:26.78 -01:42:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.735 3118286620726617088 095.61146393470 -01.71725039683 13.3380 12.8429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291958_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 291958_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292025_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292025_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:50.20 -05:15:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.807 3058473806655356928 109.70906400881 -05.25524529241 13.4385 13.2610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292031_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292031_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:44:26.07 -06:06:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.699 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292042_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292042_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:48:31.69 -04:05:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292044_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292044_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:42:39.08 -02:16:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292050_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292050_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:51:45.36 +00:25:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 4.397 3113575488282576768 102.93902775903 +00.43038993856 13.4408 13.0245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292054_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292054_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:29:26.72 -03:40:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.955 3105027919246417664 097.36147384592 -03.67625626983 13.4511 12.6576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292073_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292073_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292090_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292090_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:35:50.38 +00:49:55.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292091_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292091_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:10:08.94 +02:19:59.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292092_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292092_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:15:07.29 +02:40:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292095_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292095_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292097_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292097_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292107_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292107_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:04.47 -05:42:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292124_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292124_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292144_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292144_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292151_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292151_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292224_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292224_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292227_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292227_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:34:09.32 -00:32:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.231 3119224229266078336 098.53855094837 -00.54001848259 13.4778 12.5108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292238_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292238_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:06.46 -03:14:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.987 3059901071527241728 110.27785224367 -03.24709950855 13.5191 12.7858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292245_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292245_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:29:32.86 -02:51:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292256_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292256_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:47:10.36 -05:37:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292283_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292283_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:25.28 -03:35:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292337_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292337_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292344_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292344_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:06.98 +01:40:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.222 3114693863405107840 106.77860669604 +01.66587278863 13.6698 13.1945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292374_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292374_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292399_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292399_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:32:41.67 +01:49:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292411_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292411_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:45.13 -05:40:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.961 3059140419940666240 107.93738751668 -05.66997036834 13.7391 13.2570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292434_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292434_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:48:20.48 -00:31:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292443_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292443_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292452_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292452_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:29.24 -03:39:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292479_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292479_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:13.55 +00:52:50.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292552_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292552_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:58:20.10 -00:33:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.758 3112460446052150272 104.58351260441 -00.55517285309 13.8225 13.3508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292566_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292566_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292582_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292582_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:39:32.26 +03:12:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.184 3127159061087972864 099.88415792470 +03.20149092640 13.6964 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292583_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292583_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:58:39.83 -06:20:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:31:36.86 +00:48:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.271 3120722382580331520 097.90368843308 +00.81018091994 13.6357 13.0094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292630_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292630_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292632_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292632_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292641_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292641_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:10:42.61 -01:49:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.675 3108561474741535360 107.67777569414 -01.82779928472 13.8012 13.5079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292643_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292643_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292670_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292670_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292688_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292688_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:48:33.19 +01:51:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.281 3126156100326316672 102.13887908049 +01.85185846155 13.5491 12.7408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292702_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292702_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:44.59 -06:43:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292720_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292720_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:21:10.29 -02:12:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292733_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292733_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:13:56.24 +01:32:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292740_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292740_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292741_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292741_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292742_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292742_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:37.09 +02:26:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.293 3126439911764580096 101.65516521375 +02.44447897807 13.6481 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292745_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292745_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:50.51 +01:18:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.135 3125737976669232256 101.71061901697 +01.30128313633 13.9023 13.1882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 292802_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292802_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292810_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292810_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292821_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292821_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:33.16 +01:14:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292827_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292827_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:55.47 -03:46:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292873_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292873_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:48:20.97 -03:11:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292899_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292899_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:17:28.72 -01:37:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292903_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292903_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:04:04.94 -02:22:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.740 3108833221613004800 106.02064200889 -02.37978674497 13.9010 13.5534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292904_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292904_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292912_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292912_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292933_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292933_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:24:33.44 -01:26:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292955_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292955_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292959_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292959_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:06.12 -02:02:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.139 3108449358914585856 107.77524938523 -02.04142773742 13.6216 13.1566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292961_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292961_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292964_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292964_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292976_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292976_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:15:21.87 -00:32:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292994_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292994_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 292995_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 292995_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 292999_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 292999_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:38:18.00 -06:45:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.376 3100097640389269248 099.57433748949 -06.75730169050 13.6657 12.8453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293001_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293001_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:05:57.54 +02:49:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.150 3116003347394333696 106.49042808236 +02.82051758828 13.9886 13.5116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293040_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293040_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293058_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293058_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:58:50.11 -04:41:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.121 3101679906339288704 104.70859973578 -04.68774296413 13.8134 13.3106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293067_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293067_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293091_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293091_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:53.29 +03:13:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.908 3127291139925000832 100.97237071891 +03.21786171975 13.5859 12.7087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293095_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293095_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293134_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293134_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:32.57 +01:54:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293135_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293135_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:24:04.98 +02:32:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293137_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293137_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:35:41.98 +03:11:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.129 3130161170208610688 098.92490276050 +03.18629758406 13.7622 13.1813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293182_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293182_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:28:11.63 +01:54:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293187_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293187_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293190_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293190_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293212_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293212_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:24:37.28 +01:48:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293217_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293217_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:47:06.83 +01:33:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.693 3125769140951396608 101.77770849888 +01.56143873464 13.8938 13.1197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293228_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293228_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:59.71 +00:10:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.053 3113319370792412800 103.74872486234 +00.18032112282 13.8383 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293246_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293246_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293254_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293254_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:45.98 -00:21:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 4.332 3111161544862117376 107.44144857121 -00.35527919213 13.8352 12.8859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293269_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293269_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:37:33.22 +01:24:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.813 3120687370005889280 099.38804092931 +01.40995382945 13.9336 13.3825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293321_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293321_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:25.97 -01:49:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293330_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293330_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:54.56 +00:45:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.101 3111384127245493376 107.97730601618 +00.76008378136 13.7155 13.3460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293343_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293343_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:14:17.47 -04:07:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.891 3059549129027878528 108.57278260456 -04.13346977507 13.6768 12.9409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293345_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293345_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:39.43 -01:21:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.661 3109339619737041536 107.41478777276 -01.36419332163 13.8942 13.1712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293367_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293367_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:36.90 -04:25:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293381_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293381_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:30:13.48 -05:57:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293386_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293386_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:49:24.59 -00:56:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293442_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293442_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293455_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293455_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293491_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293491_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:16:37.39 -05:50:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293521_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293521_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 293531_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293531_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:41:27.09 -01:19:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293543_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293543_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:51:34.26 -01:39:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293558_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293558_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293569_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293569_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:39:08.65 -03:48:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.351 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293580_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293580_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:51.35 -02:54:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 4.205 3108661530301553152 105.96319311778 -02.91418890016 13.9534 13.3027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293591_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293591_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293595_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293651_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293651_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293660_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293660_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:00:54.87 +00:08:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.037 3112896368052755200 105.22787396054 +00.14609736366 13.8402 13.0240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293665_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293665_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293666_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293666_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293672_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293672_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293717_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293717_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:35:21.47 -05:17:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293719_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293719_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293785_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293785_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:04:45.76 -01:37:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.378 3109460806533000320 106.19109724512 -01.61800116054 14.0008 13.0721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293788_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293788_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:30:07.12 -02:39:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.667 3117217616247602048 097.52997534566 -02.66519300427 14.0065 13.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293819_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293819_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293830_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293830_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293844_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293844_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293849_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293849_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293854_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293854_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:20:16.25 -01:58:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.775 3109772552442329088 110.06730736101 -01.98023676963 14.1724 13.5272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293872_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293872_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:11:51.99 +02:28:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293894_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293894_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293911_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293911_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293912_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293912_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:07:52.89 +01:08:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.092 3114472346170617472 106.97045649095 +01.14911711408 13.8927 13.1411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 293919_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293919_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293935_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 293935_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 293967_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 293967_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:01.19 -00:33:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.790 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294014_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294014_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294039_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294039_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294132_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294132_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294134_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294134_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294138_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294138_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294171_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294171_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:38:52.47 +01:12:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294214_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294214_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:51:31.78 +02:21:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.212 3126292336688152960 102.88280762511 +02.35264716426 14.2305 13.3465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294345_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294345_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:39.57 -00:16:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.828 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294362_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294362_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:43:09.77 -02:13:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294413_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294413_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294425_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294425_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:26.76 -01:47:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.022 3106835550722792576 100.11111020367 -01.80053406046 14.3775 13.7940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294436_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294436_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:40:22.38 +01:18:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.708 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294449_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294449_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:05.43 +00:26:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.850 3113574212670621312 103.02253647099 +00.43546193990 13.6562 12.5960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294511_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294511_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:50.96 -02:20:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294518_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294518_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:35.48 -00:48:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.454 3112578162515589760 105.39724095265 -00.80783877429 14.1459 13.7567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294528_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294528_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:18:39.17 -01:16:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294553_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294553_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:37.00 -01:46:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 294575_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294575_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294618_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294618_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:39:21.98 -04:11:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.402 3104000459989380352 099.84229353271 -04.18904210370 14.5055 13.7184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294647_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294647_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:01:55.03 +01:12:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.260 3115365080896102400 105.47913407559 +01.21276961582 14.3007 13.4335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294653_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294653_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294675_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294675_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294677_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294677_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:02:49.03 -01:46:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.487 3109088175171141632 105.70361971433 -01.77817000677 14.4731 14.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294686_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294686_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294699_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294699_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294701_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294701_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294708_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294708_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294754_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294754_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294779_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294779_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:06:58.19 +02:05:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.333 3114788215246409088 106.74201411688 +02.09671466542 14.4155 13.6818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294780_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294780_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:08:38.35 -04:22:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.211 3107523467049454976 107.15961497013 -04.37408826363 14.5001 13.6895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294786_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294786_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:37:50.33 +03:06:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.005 3127147997252334336 099.45967977013 +03.11269445878 14.5804 13.7395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294822_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294822_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:08:40.10 -02:15:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 4.432 3108429945662948096 107.16624268895 -02.26090009078 14.6706 14.3007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294833_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294833_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:41:27.28 -01:19:23.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)
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Considering the candidate 294836_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294836_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294843_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294843_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:39:18.06 -00:00:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.289 3119634037865932160 099.82526587339 -00.01402463254 14.4432 13.6701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294948_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294948_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:54:51.85 +01:58:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.193 3114201866310760448 103.71629089400 +01.97027901056 14.5521 13.9247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294949_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294949_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:52:10.33 -01:18:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.715 3112345959404493568 103.04308562650 -01.30264108158 14.5757 13.8917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 294958_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 294958_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 294985_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 294985_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:46:39.49 -05:23:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.896 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 121122_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 121122_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:09:13.67 -02:21:30.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 65114_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 65114_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:27:01.29 -04:35:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 228912_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 06:50:00.73 +01:46:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.102 3126143833899577984 102.50251175252 +01.77583767395 10.7644 9.3430 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 43402_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 43402_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:12:52.05 -05:20:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 199360_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 246364_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 270041_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
Preparing report for the candidate 270041_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
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Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 129229_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:19:38.87 -02:00:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027
The candidate 09353_fd_Mon-02-Q1b1x1_2026-04-09_23-11-10_20.00sec_-4.90C_LIGHTs_0027 did not pass the final checks
**** FOUND 07:03:53.08 -06:53:23.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 376s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:09:13.69 -02:21:30.7
07:08:45.27 +00:41:48.4
07:17:31.28 +01:05:38.9
07:12:50.75 -04:28:36.4
06:47:33.26 -03:16:17.2
06:59:24.10 -01:09:44.4
06:56:02.36 -03:32:57.5
06:51:18.67 +02:12:26.3
06:41:50.98 +00:38:40.9
07:07:19.18 -02:52:52.0
06:45:13.01 -00:39:25.4
06:44:31.31 +01:50:52.1
06:45:34.74 -03:39:04.9
06:51:10.22 -02:40:56.1
06:56:11.45 +01:42:21.0
07:10:47.33 -05:10:04.0
07:00:42.89 -00:59:20.9
07:18:38.78 +01:25:04.3
07:00:46.38 +02:09:05.9
07:20:46.49 -01:56:42.1
06:57:02.84 +01:44:04.4
06:55:09.69 -01:33:31.9
06:53:43.60 -01:58:39.3
07:10:10.82 -03:03:00.5
06:46:25.46 +00:47:28.7
06:52:17.30 -04:22:35.3
07:16:10.37 +00:11:31.6
07:21:21.06 +00:37:47.3
06:41:26.77 +02:47:59.4
06:43:14.38 +01:58:20.7
07:06:25.75 -00:11:53.9
07:20:22.18 +01:19:59.5
07:04:05.54 +00:58:05.2
07:02:01.16 -00:36:15.8
07:00:26.40 -01:15:01.7
06:56:16.94 +00:50:21.5
07:04:56.79 -03:11:57.3
07:21:12.81 -01:21:21.0
06:53:33.70 -00:32:05.3
06:51:40.43 -01:45:27.9
07:10:18.64 -02:08:38.0
07:22:53.30 +00:28:46.1
07:04:08.11 +01:01:43.6
07:01:00.21 -05:14:06.3
06:58:34.99 -05:15:53.5
07:10:02.32 -00:20:50.0
07:20:10.15 +02:05:22.0
07:14:04.89 -05:06:36.8
06:45:23.12 +01:58:35.6
07:19:46.12 -00:10:21.1
07:08:44.81 +02:04:42.8
06:54:23.48 -04:11:23.9
07:05:45.95 +01:40:01.8
07:12:17.15 -02:10:58.9
07:10:57.94 -03:23:45.3
07:06:45.20 +00:56:41.6
07:06:31.67 +01:08:40.4
07:18:48.66 -01:43:48.0
06:42:34.58 -00:18:23.9
07:19:37.53 -02:20:14.5
07:09:41.08 -04:22:44.8
06:46:48.99 -00:40:03.3
07:18:11.90 -02:02:26.1
06:28:32.35 -00:56:47.7
07:13:31.36 -03:31:15.7
07:10:40.15 +01:18:14.0
07:08:04.41 -01:43:39.7
07:07:22.93 -06:11:24.7
07:07:04.60 -03:10:05.6
06:41:44.15 +00:27:31.4
07:14:33.99 -00:57:34.0
07:07:24.38 +02:31:25.2
07:08:02.77 -03:23:36.3
07:00:51.44 +01:33:16.4
06:40:43.72 -01:24:10.7
07:14:01.97 -01:05:42.9
07:21:07.57 -04:53:39.9
07:07:09.39 -01:15:17.2
07:09:57.91 +00:39:41.6
07:11:23.77 -00:34:13.4
07:14:12.56 -04:31:51.3
07:18:52.34 -00:04:30.1
06:57:55.16 -04:37:47.6
07:00:51.95 +00:11:59.7
07:21:01.51 -02:09:42.8
06:51:28.82 +01:57:03.4
06:41:43.37 -01:05:56.9
07:17:04.20 -04:46:10.5
07:10:56.60 -04:18:48.2
06:44:34.07 -01:35:28.8
07:13:29.35 -04:08:40.0
06:54:52.31 -02:23:38.9
06:39:15.85 +02:14:46.2
07:11:19.81 -02:24:43.4
07:09:20.58 +02:38:45.1
06:45:04.81 +02:50:46.9
07:16:34.00 -05:05:59.0
06:44:24.51 +01:59:00.0
06:40:55.24 +00:01:27.2
07:02:21.40 -04:03:31.5
07:06:44.61 -01:25:53.6
06:53:11.72 -01:33:37.3
07:11:40.11 -02:06:06.0
07:03:50.34 +01:11:51.3
07:17:51.18 -01:41:37.1
06:38:27.87 +00:48:37.5
06:48:15.49 +01:46:17.0
06:51:39.65 +00:25:33.5
07:08:35.57 +01:46:44.1
06:44:27.19 +02:30:55.2
06:40:30.43 -01:04:41.9
07:17:52.78 +00:17:03.6
07:15:49.71 -00:37:00.9
06:35:26.30 -00:39:36.5
06:34:10.96 -00:21:48.4
07:13:04.68 -05:12:23.0
07:18:20.68 -04:33:01.4
07:05:14.70 +00:02:16.4
07:20:04.46 +02:28:14.9
07:22:02.26 +00:44:40.3
07:12:56.93 +00:52:06.8
07:13:03.19 -04:47:14.4
07:10:20.76 -04:08:51.7
07:20:08.08 +01:08:58.3
07:07:33.19 -03:25:30.1
06:42:33.08 -03:28:08.0
06:44:16.44 -00:10:04.2
07:16:03.97 +02:09:51.2
07:00:50.75 -00:35:33.2
06:56:36.52 +02:42:44.7
07:03:36.83 +02:37:10.8
07:20:50.35 -00:51:21.6
07:06:24.08 -07:01:31.7
07:10:06.05 +01:43:43.2
06:46:09.07 +02:40:04.7
07:09:04.94 -02:57:19.1
07:10:07.64 +00:56:30.9
07:05:20.43 +02:45:54.2
07:04:46.59 +02:30:42.0
07:04:16.73 -03:01:38.9
06:30:03.33 +01:18:35.1
07:10:24.68 +02:20:18.2
06:57:12.28 -03:57:45.2
07:16:06.29 +00:05:10.9
06:49:53.05 +02:30:13.4
06:50:59.40 +00:13:39.3
06:49:07.02 -01:40:16.5
06:57:16.66 -06:36:37.5
07:09:31.07 -03:28:28.4
06:35:11.70 -03:04:42.8
06:54:39.39 +02:38:02.5
06:45:09.35 +02:51:07.2
06:42:44.25 +01:39:55.5
06:35:47.87 +00:35:27.0
06:48:53.05 +01:49:30.7
06:52:47.60 -06:19:15.7
06:36:32.36 -03:35:56.5
06:39:05.72 +02:23:37.7
06:57:35.66 +01:13:53.1
06:54:26.52 +02:55:35.0
06:38:41.58 +01:56:35.7
06:40:56.90 -04:34:48.5
06:48:56.91 -03:30:58.3
06:41:56.22 +00:16:59.1
07:03:45.94 -02:09:36.9
07:03:53.51 -02:54:01.8
06:49:53.84 +01:06:19.3
07:12:41.81 -00:50:01.0
06:47:59.54 -01:20:54.2
07:22:06.58 -01:59:31.9
06:52:06.42 -01:18:22.2
06:43:02.49 -04:16:55.2
07:12:56.45 -03:02:53.5
06:47:11.83 +00:21:19.8
06:49:15.96 -01:35:40.4
06:38:31.29 +02:25:41.1
07:19:41.67 -05:36:21.8
06:42:30.87 -06:04:22.2
07:12:32.61 +01:13:02.9
07:01:15.42 -00:32:58.6
06:55:11.26 -05:51:21.7
06:55:50.50 -02:12:28.5
06:53:52.16 -02:12:23.3
06:38:53.45 -00:49:17.5
07:16:17.57 +00:47:57.0
06:43:53.66 +01:01:54.3
06:44:45.96 -02:03:54.1
06:37:47.04 +01:08:57.5
07:05:42.70 -01:37:20.9
07:16:26.69 -00:01:00.2
06:45:15.21 -00:22:56.2
06:55:32.12 +01:33:42.3
07:01:01.51 +01:28:09.5
06:40:42.70 +00:45:54.0
06:59:17.83 -01:38:33.5
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
07:09:13.69 -02:21:30.7
06:47:33.26 -03:16:17.2
06:59:24.10 -01:09:44.4
06:56:02.36 -03:32:57.5
06:51:18.67 +02:12:26.3
06:41:50.98 +00:38:40.9
07:07:19.18 -02:52:52.0
06:45:13.01 -00:39:25.4
06:44:31.31 +01:50:52.1
06:45:34.74 -03:39:04.9
06:51:10.22 -02:40:56.1
06:56:11.45 +01:42:21.0
07:10:47.33 -05:10:04.0
07:00:42.89 -00:59:20.9
07:18:38.78 +01:25:04.3
07:00:46.38 +02:09:05.9
07:20:46.49 -01:56:42.1
06:57:02.84 +01:44:04.4
06:55:09.69 -01:33:31.9
06:53:43.60 -01:58:39.3
07:10:10.82 -03:03:00.5
06:46:25.46 +00:47:28.7
06:52:17.30 -04:22:35.3
07:16:10.37 +00:11:31.6
07:21:21.06 +00:37:47.3
06:41:26.77 +02:47:59.4
06:43:14.38 +01:58:20.7
07:06:25.75 -00:11:53.9
07:20:22.18 +01:19:59.5
07:04:05.54 +00:58:05.2
07:02:01.16 -00:36:15.8
07:00:26.40 -01:15:01.7
06:56:16.94 +00:50:21.5
07:04:56.79 -03:11:57.3
07:21:12.81 -01:21:21.0
06:53:33.70 -00:32:05.3
06:51:40.43 -01:45:27.9
07:10:18.64 -02:08:38.0
07:22:53.30 +00:28:46.1
07:04:08.11 +01:01:43.6
07:01:00.21 -05:14:06.3
06:58:34.99 -05:15:53.5
07:10:02.32 -00:20:50.0
07:20:10.15 +02:05:22.0
07:14:04.89 -05:06:36.8
06:45:23.12 +01:58:35.6
07:19:46.12 -00:10:21.1
07:08:44.81 +02:04:42.8
06:54:23.48 -04:11:23.9
07:05:45.95 +01:40:01.8
07:12:17.15 -02:10:58.9
07:10:57.94 -03:23:45.3
07:06:45.20 +00:56:41.6
07:06:31.67 +01:08:40.4
07:18:48.66 -01:43:48.0
06:42:34.58 -00:18:23.9
07:19:37.53 -02:20:14.5
07:09:41.08 -04:22:44.8
06:46:48.99 -00:40:03.3
07:18:11.90 -02:02:26.1
06:28:32.35 -00:56:47.7
07:13:31.36 -03:31:15.7
07:10:40.15 +01:18:14.0
07:08:04.41 -01:43:39.7
07:07:22.93 -06:11:24.7
07:07:04.60 -03:10:05.6
06:41:44.15 +00:27:31.4
07:14:33.99 -00:57:34.0
07:07:24.38 +02:31:25.2
07:08:02.77 -03:23:36.3
07:00:51.44 +01:33:16.4
06:40:43.72 -01:24:10.7
07:14:01.97 -01:05:42.9
07:21:07.57 -04:53:39.9
07:07:09.39 -01:15:17.2
07:09:57.91 +00:39:41.6
07:11:23.77 -00:34:13.4
07:14:12.56 -04:31:51.3
07:18:52.34 -00:04:30.1
06:57:55.16 -04:37:47.6
07:00:51.95 +00:11:59.7
07:21:01.51 -02:09:42.8
06:51:28.82 +01:57:03.4
06:41:43.37 -01:05:56.9
07:17:04.20 -04:46:10.5
07:10:56.60 -04:18:48.2
06:44:34.07 -01:35:28.8
07:13:29.35 -04:08:40.0
06:54:52.31 -02:23:38.9
06:39:15.85 +02:14:46.2
07:11:19.81 -02:24:43.4
07:09:20.58 +02:38:45.1
06:45:04.81 +02:50:46.9
07:16:34.00 -05:05:59.0
06:44:24.51 +01:59:00.0
06:40:55.24 +00:01:27.2
07:02:21.40 -04:03:31.5
07:06:44.61 -01:25:53.6
06:53:11.72 -01:33:37.3
07:11:40.11 -02:06:06.0
07:03:50.34 +01:11:51.3
07:17:51.18 -01:41:37.1
06:38:27.87 +00:48:37.5
06:48:15.49 +01:46:17.0
06:51:39.65 +00:25:33.5
07:08:35.57 +01:46:44.1
06:44:27.19 +02:30:55.2
06:40:30.43 -01:04:41.9
07:17:52.78 +00:17:03.6
07:15:49.71 -00:37:00.9
06:35:26.30 -00:39:36.5
06:34:10.96 -00:21:48.4
07:13:04.68 -05:12:23.0
07:18:20.68 -04:33:01.4
07:05:14.70 +00:02:16.4
07:20:04.46 +02:28:14.9
07:22:02.26 +00:44:40.3
07:12:56.93 +00:52:06.8
07:13:03.19 -04:47:14.4
07:10:20.76 -04:08:51.7
07:20:08.08 +01:08:58.3
07:07:33.19 -03:25:30.1
06:42:33.08 -03:28:08.0
06:44:16.44 -00:10:04.2
07:16:03.97 +02:09:51.2
07:00:50.75 -00:35:33.2
06:56:36.52 +02:42:44.7
07:03:36.83 +02:37:10.8
07:20:50.35 -00:51:21.6
07:06:24.08 -07:01:31.7
07:10:06.05 +01:43:43.2
06:46:09.07 +02:40:04.7
07:09:04.94 -02:57:19.1
07:10:07.64 +00:56:30.9
07:05:20.43 +02:45:54.2
07:04:46.59 +02:30:42.0
07:04:16.73 -03:01:38.9
06:30:03.33 +01:18:35.1
07:10:24.68 +02:20:18.2
06:57:12.28 -03:57:45.2
07:16:06.29 +00:05:10.9
06:49:53.05 +02:30:13.4
06:50:59.40 +00:13:39.3
06:49:07.02 -01:40:16.5
06:57:16.66 -06:36:37.5
07:09:31.07 -03:28:28.4
06:35:11.70 -03:04:42.8
06:54:39.39 +02:38:02.5
06:45:09.35 +02:51:07.2
06:42:44.25 +01:39:55.5
06:35:47.87 +00:35:27.0
06:48:53.05 +01:49:30.7
06:52:47.60 -06:19:15.7
06:36:32.36 -03:35:56.5
06:39:05.72 +02:23:37.7
06:57:35.66 +01:13:53.1
06:54:26.52 +02:55:35.0
06:38:41.58 +01:56:35.7
06:40:56.90 -04:34:48.5
06:48:56.91 -03:30:58.3
06:41:56.22 +00:16:59.1
07:03:45.94 -02:09:36.9
07:03:53.51 -02:54:01.8
06:49:53.84 +01:06:19.3
07:12:41.81 -00:50:01.0
06:47:59.54 -01:20:54.2
07:22:06.58 -01:59:31.9
06:52:06.42 -01:18:22.2
06:43:02.49 -04:16:55.2
07:12:56.45 -03:02:53.5
06:47:11.83 +00:21:19.8
06:49:15.96 -01:35:40.4
06:38:31.29 +02:25:41.1
07:19:41.67 -05:36:21.8
06:42:30.87 -06:04:22.2
07:12:32.61 +01:13:02.9
07:01:15.42 -00:32:58.6
06:55:11.26 -05:51:21.7
06:55:50.50 -02:12:28.5
06:53:52.16 -02:12:23.3
06:38:53.45 -00:49:17.5
07:16:17.57 +00:47:57.0
06:43:53.66 +01:01:54.3
06:44:45.96 -02:03:54.1
06:37:47.04 +01:08:57.5
07:05:42.70 -01:37:20.9
07:16:26.69 -00:01:00.2
06:45:15.21 -00:22:56.2
06:55:32.12 +01:33:42.3
07:01:01.51 +01:28:09.5
06:40:42.70 +00:45:54.0
06:59:17.83 -01:38:33.5
07:08:45.27 +00:41:48.4
07:17:31.28 +01:05:38.9
07:12:50.75 -04:28:36.4
###################################################################################
07:09:13.69 -02:21:30.7 -- not an asteroid (will add it to exclusion list)
06:47:33.26 -03:16:17.2 -- not an asteroid (will add it to exclusion list)
06:59:24.10 -01:09:44.4 -- not an asteroid (will add it to exclusion list)
06:56:02.36 -03:32:57.5 -- not an asteroid (will add it to exclusion list)
06:51:18.67 +02:12:26.3 -- not an asteroid (will add it to exclusion list)
06:41:50.98 +00:38:40.9 -- not an asteroid (will add it to exclusion list)
07:07:19.18 -02:52:52.0 -- not an asteroid (will add it to exclusion list)
06:45:13.01 -00:39:25.4 -- not an asteroid (will add it to exclusion list)
06:44:31.31 +01:50:52.1 -- not an asteroid (will add it to exclusion list)
06:45:34.74 -03:39:04.9 -- not an asteroid (will add it to exclusion list)
06:51:10.22 -02:40:56.1 -- not an asteroid (will add it to exclusion list)
06:56:11.45 +01:42:21.0 -- not an asteroid (will add it to exclusion list)
07:10:47.33 -05:10:04.0 -- not an asteroid (will add it to exclusion list)
07:00:42.89 -00:59:20.9 -- not an asteroid (will add it to exclusion list)
07:18:38.78 +01:25:04.3 -- not an asteroid (will add it to exclusion list)
07:00:46.38 +02:09:05.9 -- not an asteroid (will add it to exclusion list)
07:20:46.49 -01:56:42.1 -- not an asteroid (will add it to exclusion list)
06:57:02.84 +01:44:04.4 -- not an asteroid (will add it to exclusion list)
06:55:09.69 -01:33:31.9 -- not an asteroid (will add it to exclusion list)
06:53:43.60 -01:58:39.3 -- not an asteroid (will add it to exclusion list)
07:10:10.82 -03:03:00.5 -- not an asteroid (will add it to exclusion list)
06:46:25.46 +00:47:28.7 -- not an asteroid (will add it to exclusion list)
06:52:17.30 -04:22:35.3 -- not an asteroid (will add it to exclusion list)
07:16:10.37 +00:11:31.6 -- not an asteroid (will add it to exclusion list)
07:21:21.06 +00:37:47.3 -- not an asteroid (will add it to exclusion list)
06:41:26.77 +02:47:59.4 -- not an asteroid (will add it to exclusion list)
06:43:14.38 +01:58:20.7 -- not an asteroid (will add it to exclusion list)
07:06:25.75 -00:11:53.9 -- not an asteroid (will add it to exclusion list)
07:20:22.18 +01:19:59.5 -- not an asteroid (will add it to exclusion list)
07:04:05.54 +00:58:05.2 -- not an asteroid (will add it to exclusion list)
07:02:01.16 -00:36:15.8 -- not an asteroid (will add it to exclusion list)
07:00:26.40 -01:15:01.7 -- not an asteroid (will add it to exclusion list)
06:56:16.94 +00:50:21.5 -- not an asteroid (will add it to exclusion list)
07:04:56.79 -03:11:57.3 -- not an asteroid (will add it to exclusion list)
07:21:12.81 -01:21:21.0 -- not an asteroid (will add it to exclusion list)
06:53:33.70 -00:32:05.3 -- not an asteroid (will add it to exclusion list)
06:51:40.43 -01:45:27.9 -- not an asteroid (will add it to exclusion list)
07:10:18.64 -02:08:38.0 -- not an asteroid (will add it to exclusion list)
07:22:53.30 +00:28:46.1 -- not an asteroid (will add it to exclusion list)
07:04:08.11 +01:01:43.6 -- not an asteroid (will add it to exclusion list)
07:01:00.21 -05:14:06.3 -- not an asteroid (will add it to exclusion list)
06:58:34.99 -05:15:53.5 -- not an asteroid (will add it to exclusion list)
07:10:02.32 -00:20:50.0 -- not an asteroid (will add it to exclusion list)
07:20:10.15 +02:05:22.0 -- not an asteroid (will add it to exclusion list)
07:14:04.89 -05:06:36.8 -- not an asteroid (will add it to exclusion list)
06:45:23.12 +01:58:35.6 -- not an asteroid (will add it to exclusion list)
07:19:46.12 -00:10:21.1 -- not an asteroid (will add it to exclusion list)
07:08:44.81 +02:04:42.8 -- not an asteroid (will add it to exclusion list)
06:54:23.48 -04:11:23.9 -- not an asteroid (will add it to exclusion list)
07:05:45.95 +01:40:01.8 -- not an asteroid (will add it to exclusion list)
07:12:17.15 -02:10:58.9 -- not an asteroid (will add it to exclusion list)
07:10:57.94 -03:23:45.3 -- not an asteroid (will add it to exclusion list)
07:06:45.20 +00:56:41.6 -- not an asteroid (will add it to exclusion list)
07:06:31.67 +01:08:40.4 -- not an asteroid (will add it to exclusion list)
07:18:48.66 -01:43:48.0 -- not an asteroid (will add it to exclusion list)
06:42:34.58 -00:18:23.9 -- not an asteroid (will add it to exclusion list)
07:19:37.53 -02:20:14.5 -- not an asteroid (will add it to exclusion list)
07:09:41.08 -04:22:44.8 -- not an asteroid (will add it to exclusion list)
06:46:48.99 -00:40:03.3 -- not an asteroid (will add it to exclusion list)
07:18:11.90 -02:02:26.1 -- not an asteroid (will add it to exclusion list)
06:28:32.35 -00:56:47.7 -- not an asteroid (will add it to exclusion list)
07:13:31.36 -03:31:15.7 -- not an asteroid (will add it to exclusion list)
07:10:40.15 +01:18:14.0 -- not an asteroid (will add it to exclusion list)
07:08:04.41 -01:43:39.7 -- not an asteroid (will add it to exclusion list)
07:07:22.93 -06:11:24.7 -- not an asteroid (will add it to exclusion list)
07:07:04.60 -03:10:05.6 -- not an asteroid (will add it to exclusion list)
06:41:44.15 +00:27:31.4 -- not an asteroid (will add it to exclusion list)
07:14:33.99 -00:57:34.0 -- not an asteroid (will add it to exclusion list)
07:07:24.38 +02:31:25.2 -- not an asteroid (will add it to exclusion list)
07:08:02.77 -03:23:36.3 -- not an asteroid (will add it to exclusion list)
07:00:51.44 +01:33:16.4 -- not an asteroid (will add it to exclusion list)
06:40:43.72 -01:24:10.7 -- not an asteroid (will add it to exclusion list)
07:14:01.97 -01:05:42.9 -- not an asteroid (will add it to exclusion list)
07:21:07.57 -04:53:39.9 -- not an asteroid (will add it to exclusion list)
07:07:09.39 -01:15:17.2 -- not an asteroid (will add it to exclusion list)
07:09:57.91 +00:39:41.6 -- not an asteroid (will add it to exclusion list)
07:11:23.77 -00:34:13.4 -- not an asteroid (will add it to exclusion list)
07:14:12.56 -04:31:51.3 -- not an asteroid (will add it to exclusion list)
07:18:52.34 -00:04:30.1 -- not an asteroid (will add it to exclusion list)
06:57:55.16 -04:37:47.6 -- not an asteroid (will add it to exclusion list)
07:00:51.95 +00:11:59.7 -- not an asteroid (will add it to exclusion list)
07:21:01.51 -02:09:42.8 -- not an asteroid (will add it to exclusion list)
06:51:28.82 +01:57:03.4 -- not an asteroid (will add it to exclusion list)
06:41:43.37 -01:05:56.9 -- not an asteroid (will add it to exclusion list)
07:17:04.20 -04:46:10.5 -- not an asteroid (will add it to exclusion list)
07:10:56.60 -04:18:48.2 -- not an asteroid (will add it to exclusion list)
06:44:34.07 -01:35:28.8 -- not an asteroid (will add it to exclusion list)
07:13:29.35 -04:08:40.0 -- not an asteroid (will add it to exclusion list)
06:54:52.31 -02:23:38.9 -- not an asteroid (will add it to exclusion list)
06:39:15.85 +02:14:46.2 -- not an asteroid (will add it to exclusion list)
07:11:19.81 -02:24:43.4 -- not an asteroid (will add it to exclusion list)
07:09:20.58 +02:38:45.1 -- not an asteroid (will add it to exclusion list)
06:45:04.81 +02:50:46.9 -- not an asteroid (will add it to exclusion list)
07:16:34.00 -05:05:59.0 -- not an asteroid (will add it to exclusion list)
06:44:24.51 +01:59:00.0 -- not an asteroid (will add it to exclusion list)
06:40:55.24 +00:01:27.2 -- not an asteroid (will add it to exclusion list)
07:02:21.40 -04:03:31.5 -- not an asteroid (will add it to exclusion list)
07:06:44.61 -01:25:53.6 -- not an asteroid (will add it to exclusion list)
06:53:11.72 -01:33:37.3 -- not an asteroid (will add it to exclusion list)
07:11:40.11 -02:06:06.0 -- not an asteroid (will add it to exclusion list)
07:03:50.34 +01:11:51.3 -- not an asteroid (will add it to exclusion list)
07:17:51.18 -01:41:37.1 -- not an asteroid (will add it to exclusion list)
06:38:27.87 +00:48:37.5 -- not an asteroid (will add it to exclusion list)
06:48:15.49 +01:46:17.0 -- not an asteroid (will add it to exclusion list)
06:51:39.65 +00:25:33.5 -- not an asteroid (will add it to exclusion list)
07:08:35.57 +01:46:44.1 -- not an asteroid (will add it to exclusion list)
06:44:27.19 +02:30:55.2 -- not an asteroid (will add it to exclusion list)
06:40:30.43 -01:04:41.9 -- not an asteroid (will add it to exclusion list)
07:17:52.78 +00:17:03.6 -- not an asteroid (will add it to exclusion list)
07:15:49.71 -00:37:00.9 -- not an asteroid (will add it to exclusion list)
06:35:26.30 -00:39:36.5 -- not an asteroid (will add it to exclusion list)
06:34:10.96 -00:21:48.4 -- not an asteroid (will add it to exclusion list)
07:13:04.68 -05:12:23.0 -- not an asteroid (will add it to exclusion list)
07:18:20.68 -04:33:01.4 -- not an asteroid (will add it to exclusion list)
07:05:14.70 +00:02:16.4 -- not an asteroid (will add it to exclusion list)
07:20:04.46 +02:28:14.9 -- not an asteroid (will add it to exclusion list)
07:22:02.26 +00:44:40.3 -- not an asteroid (will add it to exclusion list)
07:12:56.93 +00:52:06.8 -- not an asteroid (will add it to exclusion list)
07:13:03.19 -04:47:14.4 -- not an asteroid (will add it to exclusion list)
07:10:20.76 -04:08:51.7 -- not an asteroid (will add it to exclusion list)
07:20:08.08 +01:08:58.3 -- not an asteroid (will add it to exclusion list)
07:07:33.19 -03:25:30.1 -- not an asteroid (will add it to exclusion list)
06:42:33.08 -03:28:08.0 -- not an asteroid (will add it to exclusion list)
06:44:16.44 -00:10:04.2 -- not an asteroid (will add it to exclusion list)
07:16:03.97 +02:09:51.2 -- not an asteroid (will add it to exclusion list)
07:00:50.75 -00:35:33.2 -- not an asteroid (will add it to exclusion list)
06:56:36.52 +02:42:44.7 -- not an asteroid (will add it to exclusion list)
07:03:36.83 +02:37:10.8 -- not an asteroid (will add it to exclusion list)
07:20:50.35 -00:51:21.6 -- not an asteroid (will add it to exclusion list)
07:06:24.08 -07:01:31.7 -- not an asteroid (will add it to exclusion list)
07:10:06.05 +01:43:43.2 -- not an asteroid (will add it to exclusion list)
06:46:09.07 +02:40:04.7 -- not an asteroid (will add it to exclusion list)
07:09:04.94 -02:57:19.1 -- not an asteroid (will add it to exclusion list)
07:10:07.64 +00:56:30.9 -- not an asteroid (will add it to exclusion list)
07:05:20.43 +02:45:54.2 -- not an asteroid (will add it to exclusion list)
07:04:46.59 +02:30:42.0 -- not an asteroid (will add it to exclusion list)
07:04:16.73 -03:01:38.9 -- not an asteroid (will add it to exclusion list)
06:30:03.33 +01:18:35.1 -- not an asteroid (will add it to exclusion list)
07:10:24.68 +02:20:18.2 -- not an asteroid (will add it to exclusion list)
06:57:12.28 -03:57:45.2 -- not an asteroid (will add it to exclusion list)
07:16:06.29 +00:05:10.9 -- not an asteroid (will add it to exclusion list)
06:49:53.05 +02:30:13.4 -- not an asteroid (will add it to exclusion list)
06:50:59.40 +00:13:39.3 -- not an asteroid (will add it to exclusion list)
06:49:07.02 -01:40:16.5 -- not an asteroid (will add it to exclusion list)
06:57:16.66 -06:36:37.5 -- not an asteroid (will add it to exclusion list)
07:09:31.07 -03:28:28.4 -- not an asteroid (will add it to exclusion list)
06:35:11.70 -03:04:42.8 -- not an asteroid (will add it to exclusion list)
06:54:39.39 +02:38:02.5 -- not an asteroid (will add it to exclusion list)
06:45:09.35 +02:51:07.2 -- not an asteroid (will add it to exclusion list)
06:42:44.25 +01:39:55.5 -- not an asteroid (will add it to exclusion list)
06:35:47.87 +00:35:27.0 -- not an asteroid (will add it to exclusion list)
06:48:53.05 +01:49:30.7 -- not an asteroid (will add it to exclusion list)
06:52:47.60 -06:19:15.7 -- not an asteroid (will add it to exclusion list)
06:36:32.36 -03:35:56.5 -- not an asteroid (will add it to exclusion list)
06:39:05.72 +02:23:37.7 -- not an asteroid (will add it to exclusion list)
06:57:35.66 +01:13:53.1 -- not an asteroid (will add it to exclusion list)
06:54:26.52 +02:55:35.0 -- not an asteroid (will add it to exclusion list)
06:38:41.58 +01:56:35.7 -- not an asteroid (will add it to exclusion list)
06:40:56.90 -04:34:48.5 -- not an asteroid (will add it to exclusion list)
06:48:56.91 -03:30:58.3 -- not an asteroid (will add it to exclusion list)
06:41:56.22 +00:16:59.1 -- not an asteroid (will add it to exclusion list)
07:03:45.94 -02:09:36.9 -- not an asteroid (will add it to exclusion list)
07:03:53.51 -02:54:01.8 -- not an asteroid (will add it to exclusion list)
06:49:53.84 +01:06:19.3 -- not an asteroid (will add it to exclusion list)
07:12:41.81 -00:50:01.0 -- not an asteroid (will add it to exclusion list)
06:47:59.54 -01:20:54.2 -- not an asteroid (will add it to exclusion list)
07:22:06.58 -01:59:31.9 -- not an asteroid (will add it to exclusion list)
06:52:06.42 -01:18:22.2 -- not an asteroid (will add it to exclusion list)
06:43:02.49 -04:16:55.2 -- not an asteroid (will add it to exclusion list)
07:12:56.45 -03:02:53.5 -- not an asteroid (will add it to exclusion list)
06:47:11.83 +00:21:19.8 -- not an asteroid (will add it to exclusion list)
06:49:15.96 -01:35:40.4 -- not an asteroid (will add it to exclusion list)
06:38:31.29 +02:25:41.1 -- not an asteroid (will add it to exclusion list)
07:19:41.67 -05:36:21.8 -- not an asteroid (will add it to exclusion list)
06:42:30.87 -06:04:22.2 -- not an asteroid (will add it to exclusion list)
07:12:32.61 +01:13:02.9 -- not an asteroid (will add it to exclusion list)
07:01:15.42 -00:32:58.6 -- not an asteroid (will add it to exclusion list)
06:55:11.26 -05:51:21.7 -- not an asteroid (will add it to exclusion list)
06:55:50.50 -02:12:28.5 -- not an asteroid (will add it to exclusion list)
06:53:52.16 -02:12:23.3 -- not an asteroid (will add it to exclusion list)
06:38:53.45 -00:49:17.5 -- not an asteroid (will add it to exclusion list)
07:16:17.57 +00:47:57.0 -- not an asteroid (will add it to exclusion list)
06:43:53.66 +01:01:54.3 -- not an asteroid (will add it to exclusion list)
06:44:45.96 -02:03:54.1 -- not an asteroid (will add it to exclusion list)
06:37:47.04 +01:08:57.5 -- not an asteroid (will add it to exclusion list)
07:05:42.70 -01:37:20.9 -- not an asteroid (will add it to exclusion list)
07:16:26.69 -00:01:00.2 -- not an asteroid (will add it to exclusion list)
06:45:15.21 -00:22:56.2 -- not an asteroid (will add it to exclusion list)
06:55:32.12 +01:33:42.3 -- not an asteroid (will add it to exclusion list)
07:01:01.51 +01:28:09.5 -- not an asteroid (will add it to exclusion list)
06:40:42.70 +00:45:54.0 -- not an asteroid (will add it to exclusion list)
06:59:17.83 -01:38:33.5 -- not an asteroid (will add it to exclusion list)
07:08:45.27 +00:41:48.4 -- not an asteroid (will add it to exclusion list)
07:17:31.28 +01:05:38.9 -- not an asteroid (will add it to exclusion list)
07:12:50.75 -04:28:36.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:28:32.35 -00:56:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:03.33 +01:18:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:34:10.96 -00:21:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:11.70 -03:04:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:26.30 -00:39:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:47.87 +00:35:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:32.36 -03:35:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:47.04 +01:08:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:27.87 +00:48:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:31.29 +02:25:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:41.58 +01:56:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:53.45 -00:49:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:05.72 +02:23:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:15.85 +02:14:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:30.43 -01:04:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:42.70 +00:45:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:43.72 -01:24:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:55.24 +00:01:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:56.90 -04:34:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:26.77 +02:47:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:43.37 -01:05:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:44.15 +00:27:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:50.98 +00:38:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:56.22 +00:16:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:30.87 -06:04:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.08 -03:28:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:34.58 -00:18:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:44.25 +01:39:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:02.49 -04:16:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.38 +01:58:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:53.66 +01:01:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:16.44 -00:10:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:24.51 +01:59:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:27.19 +02:30:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:31.31 +01:50:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.07 -01:35:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:45.96 -02:03:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:04.81 +02:50:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:09.35 +02:51:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:13.01 -00:39:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:15.21 -00:22:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:23.12 +01:58:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:34.74 -03:39:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:09.07 +02:40:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:25.46 +00:47:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:48.99 -00:40:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:11.83 +00:21:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:33.26 -03:16:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.54 -01:20:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:15.49 +01:46:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:53.05 +01:49:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:56.91 -03:30:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.02 -01:40:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:15.96 -01:35:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:53.05 +02:30:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:53.84 +01:06:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.40 +00:13:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.22 -02:40:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.67 +02:12:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.82 +01:57:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:39.65 +00:25:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:40.43 -01:45:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.42 -01:18:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:17.30 -04:22:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:47.60 -06:19:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:11.72 -01:33:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:33.70 -00:32:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:43.60 -01:58:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:52.16 -02:12:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:23.48 -04:11:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:26.52 +02:55:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.39 +02:38:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:52.31 -02:23:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:09.69 -01:33:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:11.26 -05:51:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:32.12 +01:33:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.50 -02:12:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:02.36 -03:32:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:11.45 +01:42:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:16.94 +00:50:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:36.52 +02:42:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:02.84 +01:44:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.28 -03:57:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.66 -06:36:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.66 +01:13:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.16 -04:37:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.99 -05:15:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:17.83 -01:38:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:24.10 -01:09:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:26.40 -01:15:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:42.89 -00:59:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:46.38 +02:09:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:50.75 -00:35:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:51.44 +01:33:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:51.95 +00:11:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:00.21 -05:14:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:01.51 +01:28:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.42 -00:32:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:01.16 -00:36:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.40 -04:03:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.83 +02:37:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:45.94 -02:09:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:50.34 +01:11:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:53.51 -02:54:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:05.54 +00:58:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:08.11 +01:01:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.73 -03:01:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:46.59 +02:30:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:56.79 -03:11:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:14.70 +00:02:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.43 +02:45:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:42.70 -01:37:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:45.95 +01:40:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:24.08 -07:01:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:25.75 -00:11:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.67 +01:08:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:44.61 -01:25:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:45.20 +00:56:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:04.60 -03:10:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:09.39 -01:15:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:19.18 -02:52:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:22.93 -06:11:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.38 +02:31:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:33.19 -03:25:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:02.77 -03:23:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:04.41 -01:43:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:35.57 +01:46:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:44.81 +02:04:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:45.27 +00:41:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:04.94 -02:57:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.69 -02:21:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:20.58 +02:38:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:31.07 -03:28:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:41.08 -04:22:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:57.91 +00:39:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:02.32 -00:20:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:06.05 +01:43:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:07.64 +00:56:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:10.82 -03:03:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:18.64 -02:08:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:20.76 -04:08:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:24.68 +02:20:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:40.15 +01:18:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:47.33 -05:10:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:56.60 -04:18:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:57.94 -03:23:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.81 -02:24:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:23.77 -00:34:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:40.11 -02:06:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:17.15 -02:10:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:32.61 +01:13:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:41.81 -00:50:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:50.75 -04:28:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.45 -03:02:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:12:56.93 +00:52:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:03.19 -04:47:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:04.68 -05:12:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:29.35 -04:08:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:13:31.36 -03:31:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:01.97 -01:05:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:04.89 -05:06:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:12.56 -04:31:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:33.99 -00:57:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:49.71 -00:37:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:03.97 +02:09:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:06.29 +00:05:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:10.37 +00:11:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:17.57 +00:47:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:26.69 -00:01:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:16:34.00 -05:05:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:04.20 -04:46:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:31.28 +01:05:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:51.18 -01:41:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:52.78 +00:17:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:11.90 -02:02:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:20.68 -04:33:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:38.78 +01:25:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:48.66 -01:43:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:52.34 -00:04:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:37.53 -02:20:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:41.67 -05:36:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:46.12 -00:10:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:04.46 +02:28:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:08.08 +01:08:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:10.15 +02:05:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:22.18 +01:19:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:46.49 -01:56:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:20:50.35 -00:51:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:01.51 -02:09:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:07.57 -04:53:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:12.81 -01:21:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:21:21.06 +00:37:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:02.26 +00:44:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:06.58 -01:59:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:22:53.30 +00:28:46.1 -- 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)
06:28:32.35 -00:56:47.7 -- not a known variable star
06:30:03.33 +01:18:35.1 -- a known variable star
06:34:10.96 -00:21:48.4 -- not a known variable star
06:35:11.70 -03:04:42.8 -- not a known variable star
06:35:26.30 -00:39:36.5 -- not a known variable star
06:35:47.87 +00:35:27.0 -- not a known variable star
06:36:32.36 -03:35:56.5 -- not a known variable star
06:37:47.04 +01:08:57.5 -- not a known variable star
06:38:27.87 +00:48:37.5 -- a known variable star
06:38:31.29 +02:25:41.1 -- a known variable star
06:38:41.58 +01:56:35.7 -- not a known variable star
06:38:53.45 -00:49:17.5 -- not a known variable star
06:39:05.72 +02:23:37.7 -- a known variable star
06:39:15.85 +02:14:46.2 -- not a known variable star
06:40:30.43 -01:04:41.9 -- a known variable star
06:40:42.70 +00:45:54.0 -- a known variable star
06:40:43.72 -01:24:10.7 -- a known variable star
06:40:55.24 +00:01:27.2 -- a known variable star
06:40:56.90 -04:34:48.5 -- not a known variable star
06:41:26.77 +02:47:59.4 -- not a known variable star
06:41:43.37 -01:05:56.9 -- not a known variable star
06:41:44.15 +00:27:31.4 -- a known variable star
06:41:50.98 +00:38:40.9 -- not a known variable star
06:41:56.22 +00:16:59.1 -- not a known variable star
06:42:30.87 -06:04:22.2 -- a known variable star
06:42:33.08 -03:28:08.0 -- not a known variable star
06:42:34.58 -00:18:23.9 -- not a known variable star
06:42:44.25 +01:39:55.5 -- not a known variable star
06:43:02.49 -04:16:55.2 -- not a known variable star
06:43:14.38 +01:58:20.7 -- not a known variable star
06:43:53.66 +01:01:54.3 -- a known variable star
06:44:16.44 -00:10:04.2 -- not a known variable star
06:44:24.51 +01:59:00.0 -- not a known variable star
06:44:27.19 +02:30:55.2 -- not a known variable star
06:44:31.31 +01:50:52.1 -- not a known variable star
06:44:34.07 -01:35:28.8 -- a known variable star
06:44:45.96 -02:03:54.1 -- not a known variable star
06:45:04.81 +02:50:46.9 -- not a known variable star
06:45:09.35 +02:51:07.2 -- a known variable star
06:45:13.01 -00:39:25.4 -- not a known variable star
06:45:15.21 -00:22:56.2 -- not a known variable star
06:45:23.12 +01:58:35.6 -- not a known variable star
06:45:34.74 -03:39:04.9 -- not a known variable star
06:46:09.07 +02:40:04.7 -- a known variable star
06:46:25.46 +00:47:28.7 -- not a known variable star
06:46:48.99 -00:40:03.3 -- not a known variable star
06:47:11.83 +00:21:19.8 -- a known variable star
06:47:33.26 -03:16:17.2 -- a known variable star
06:47:59.54 -01:20:54.2 -- not a known variable star
06:48:15.49 +01:46:17.0 -- not a known variable star
06:48:53.05 +01:49:30.7 -- a known variable star
06:48:56.91 -03:30:58.3 -- not a known variable star
06:49:07.02 -01:40:16.5 -- not a known variable star
06:49:15.96 -01:35:40.4 -- not a known variable star
06:49:53.05 +02:30:13.4 -- a known variable star
06:49:53.84 +01:06:19.3 -- not a known variable star
06:50:59.40 +00:13:39.3 -- not a known variable star
06:51:10.22 -02:40:56.1 -- not a known variable star
06:51:18.67 +02:12:26.3 -- not a known variable star
06:51:28.82 +01:57:03.4 -- not a known variable star
06:51:39.65 +00:25:33.5 -- not a known variable star
06:51:40.43 -01:45:27.9 -- not a known variable star
06:52:06.42 -01:18:22.2 -- not a known variable star
06:52:17.30 -04:22:35.3 -- not a known variable star
06:52:47.60 -06:19:15.7 -- not a known variable star
06:53:11.72 -01:33:37.3 -- a known variable star
06:53:33.70 -00:32:05.3 -- not a known variable star
06:53:43.60 -01:58:39.3 -- not a known variable star
06:53:52.16 -02:12:23.3 -- not a known variable star
06:54:23.48 -04:11:23.9 -- not a known variable star
06:54:26.52 +02:55:35.0 -- not a known variable star
06:54:39.39 +02:38:02.5 -- not a known variable star
06:54:52.31 -02:23:38.9 -- a known variable star
06:55:09.69 -01:33:31.9 -- a known variable star
06:55:11.26 -05:51:21.7 -- not a known variable star
06:55:32.12 +01:33:42.3 -- not a known variable star
06:55:50.50 -02:12:28.5 -- not a known variable star
06:56:02.36 -03:32:57.5 -- a known variable star
06:56:11.45 +01:42:21.0 -- not a known variable star
06:56:16.94 +00:50:21.5 -- not a known variable star
06:56:36.52 +02:42:44.7 -- not a known variable star
06:57:02.84 +01:44:04.4 -- not a known variable star
06:57:12.28 -03:57:45.2 -- not a known variable star
06:57:16.66 -06:36:37.5 -- a known variable star
06:57:35.66 +01:13:53.1 -- a known variable star
06:57:55.16 -04:37:47.6 -- a known variable star
06:58:34.99 -05:15:53.5 -- a known variable star
06:59:17.83 -01:38:33.5 -- not a known variable star
06:59:24.10 -01:09:44.4 -- not a known variable star
07:00:26.40 -01:15:01.7 -- not a known variable star
07:00:42.89 -00:59:20.9 -- not a known variable star
07:00:46.38 +02:09:05.9 -- not a known variable star
07:00:50.75 -00:35:33.2 -- not a known variable star
07:00:51.44 +01:33:16.4 -- not a known variable star
07:00:51.95 +00:11:59.7 -- not a known variable star
07:01:00.21 -05:14:06.3 -- not a known variable star
07:01:01.51 +01:28:09.5 -- not a known variable star
07:01:15.42 -00:32:58.6 -- a known variable star
07:02:01.16 -00:36:15.8 -- not a known variable star
07:02:21.40 -04:03:31.5 -- a known variable star
07:03:36.83 +02:37:10.8 -- a known variable star
07:03:45.94 -02:09:36.9 -- not a known variable star
07:03:50.34 +01:11:51.3 -- a known variable star
07:03:53.51 -02:54:01.8 -- not a known variable star
07:04:05.54 +00:58:05.2 -- not a known variable star
07:04:08.11 +01:01:43.6 -- not a known variable star
07:04:16.73 -03:01:38.9 -- not a known variable star
07:04:46.59 +02:30:42.0 -- not a known variable star
07:04:56.79 -03:11:57.3 -- not a known variable star
07:05:14.70 +00:02:16.4 -- not a known variable star
07:05:20.43 +02:45:54.2 -- not a known variable star
07:05:42.70 -01:37:20.9 -- not a known variable star
07:05:45.95 +01:40:01.8 -- a known variable star
07:06:24.08 -07:01:31.7 -- not a known variable star
07:06:25.75 -00:11:53.9 -- not a known variable star
07:06:31.67 +01:08:40.4 -- a known variable star
07:06:44.61 -01:25:53.6 -- not a known variable star
07:06:45.20 +00:56:41.6 -- a known variable star
07:07:04.60 -03:10:05.6 -- not a known variable star
07:07:09.39 -01:15:17.2 -- a known variable star
07:07:19.18 -02:52:52.0 -- not a known variable star
07:07:22.93 -06:11:24.7 -- not a known variable star
07:07:24.38 +02:31:25.2 -- not a known variable star
07:07:33.19 -03:25:30.1 -- a known variable star
07:08:02.77 -03:23:36.3 -- not a known variable star
07:08:04.41 -01:43:39.7 -- not a known variable star
07:08:35.57 +01:46:44.1 -- not a known variable star
07:08:44.81 +02:04:42.8 -- a known variable star
07:08:45.27 +00:41:48.4 -- a known variable star
07:09:04.94 -02:57:19.1 -- a known variable star
07:09:13.69 -02:21:30.7 -- a known variable star
07:09:20.58 +02:38:45.1 -- not a known variable star
07:09:31.07 -03:28:28.4 -- not a known variable star
07:09:41.08 -04:22:44.8 -- not a known variable star
07:09:57.91 +00:39:41.6 -- not a known variable star
07:10:02.32 -00:20:50.0 -- not a known variable star
07:10:06.05 +01:43:43.2 -- not a known variable star
07:10:07.64 +00:56:30.9 -- not a known variable star
07:10:10.82 -03:03:00.5 -- not a known variable star
07:10:18.64 -02:08:38.0 -- not a known variable star
07:10:20.76 -04:08:51.7 -- not a known variable star
07:10:24.68 +02:20:18.2 -- not a known variable star
07:10:40.15 +01:18:14.0 -- not a known variable star
07:10:47.33 -05:10:04.0 -- not a known variable star
07:10:56.60 -04:18:48.2 -- not a known variable star
07:10:57.94 -03:23:45.3 -- a known variable star
07:11:19.81 -02:24:43.4 -- not a known variable star
07:11:23.77 -00:34:13.4 -- not a known variable star
07:11:40.11 -02:06:06.0 -- not a known variable star
07:12:17.15 -02:10:58.9 -- not a known variable star
07:12:32.61 +01:13:02.9 -- not a known variable star
07:12:41.81 -00:50:01.0 -- not a known variable star
07:12:50.75 -04:28:36.4 -- a known variable star
07:12:56.45 -03:02:53.5 -- a known variable star
07:12:56.93 +00:52:06.8 -- a known variable star
07:13:03.19 -04:47:14.4 -- not a known variable star
07:13:04.68 -05:12:23.0 -- a known variable star
07:13:29.35 -04:08:40.0 -- not a known variable star
07:13:31.36 -03:31:15.7 -- not a known variable star
07:14:01.97 -01:05:42.9 -- not a known variable star
07:14:04.89 -05:06:36.8 -- a known variable star
07:14:12.56 -04:31:51.3 -- a known variable star
07:14:33.99 -00:57:34.0 -- not a known variable star
07:15:49.71 -00:37:00.9 -- a known variable star
07:16:03.97 +02:09:51.2 -- not a known variable star
07:16:06.29 +00:05:10.9 -- a known variable star
07:16:10.37 +00:11:31.6 -- not a known variable star
07:16:17.57 +00:47:57.0 -- not a known variable star
07:16:26.69 -00:01:00.2 -- not a known variable star
07:16:34.00 -05:05:59.0 -- a known variable star
07:17:04.20 -04:46:10.5 -- not a known variable star
07:17:31.28 +01:05:38.9 -- a known variable star
07:17:51.18 -01:41:37.1 -- a known variable star
07:17:52.78 +00:17:03.6 -- a known variable star
07:18:11.90 -02:02:26.1 -- not a known variable star
07:18:20.68 -04:33:01.4 -- a known variable star
07:18:38.78 +01:25:04.3 -- not a known variable star
07:18:48.66 -01:43:48.0 -- not a known variable star
07:18:52.34 -00:04:30.1 -- not a known variable star
07:19:37.53 -02:20:14.5 -- not a known variable star
07:19:41.67 -05:36:21.8 -- not a known variable star
07:19:46.12 -00:10:21.1 -- not a known variable star
07:20:04.46 +02:28:14.9 -- not a known variable star
07:20:08.08 +01:08:58.3 -- not a known variable star
07:20:10.15 +02:05:22.0 -- a known variable star
07:20:22.18 +01:19:59.5 -- not a known variable star
07:20:46.49 -01:56:42.1 -- a known variable star
07:20:50.35 -00:51:21.6 -- a known variable star
07:21:01.51 -02:09:42.8 -- not a known variable star
07:21:07.57 -04:53:39.9 -- not a known variable star
07:21:12.81 -01:21:21.0 -- a known variable star
07:21:21.06 +00:37:47.3 -- not a known variable star
07:22:02.26 +00:44:40.3 -- not a known variable star
07:22:06.58 -01:59:31.9 -- not a known variable star
07:22:53.30 +00:28:46.1 -- a known variable star
Found 137 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
195 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 195 (excluding asteroids and hot pixels, 137 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)2461140.67372288 -observatory V36
23:38:09.82 -04:55:09.1 Mercury (0.2mag)
02:40:26.39 +15:33:10.2 Venus (-3.9mag)
00:01:16.05 -00:57:38.1 Mars (1.2mag)
07:10:10.00 +22:50:11.4 Jupiter (-2.1mag)
00:26:33.98 +00:32:36.5 Saturn (0.9mag)
03:46:30.05 +19:43:37.4 Uranus (5.8mag)
00:10:04.08 -00:20:15.1 Neptune (7.8mag)
20:33:28.09 -22:52:27.0 Pluto (14.5mag)
19:29:44.69 -26:00:32.3 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Apr 9 23:24 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461140.67372288:
07:10:03.13 +22:50:23.5 Io (5.7mag)
07:10:17.96 +22:49:52.3 Europa (5.9mag)
07:10:08.70 +22:50:06.3 Ganymede (5.3mag)
07:09:48.36 +22:51:01.6 Callisto (6.6mag)
07:13:44.57 +22:40:38.2 Himalia (15.3mag)
07:10:06.00 +22:50:20.0 Thebe (16.2mag)
07:13:48.04 +23:10:10.0 Elara (17.3mag)
07:08:39.07 +23:33:14.6 Pasiphae (17.4mag)
07:18:37.14 +22:47:35.9 Carme (18.5mag)
00:26:43.85 +00:32:27.3 Titan (8.8mag)
00:26:32.85 +00:32:52.6 Rhea (10.1mag)
00:26:25.53 +00:33:39.5 Iapetus (11.5mag)
00:26:47.50 +00:32:25.2 Hyperion (14.8mag)
00:28:15.35 +00:42:01.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 23:24 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.67372288:
15:10:00.89 -11:48:33.6 JWST
19:16:24.55 +13:55:12.2 Chandra
07:57:47.32 -37:05:38.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 23:24 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.67372288 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:19.47 -28:26:53.4 13.9mag P/2010 H2 (Vales)
05:02:40.89 -69:56:42.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:16.06 +31:23:58.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:51.32 +09:51:06.3 17.6mag C/2021 G2 (ATLAS)
23:08:35.05 +29:00:25.0 17.0mag C/2022 E2 (ATLAS)
04:22:30.41 +25:52:39.1 15.9mag C/2022 N2 (PANSTARRS)
09:02:21.23 +31:57:56.6 16.2mag C/2022 QE78 (ATLAS)
08:30:19.11 -00:47:02.3 17.3mag C/2022 R6 (PANSTARRS)
18:54:57.37 +18:02:17.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:27.06 -11:36:20.4 17.5mag P/2023 B1 (PANSTARRS)
09:10:33.18 -12:50:00.1 17.6mag C/2023 F3 (ATLAS)
21:48:03.86 +62:34:40.5 17.5mag C/2023 H5 (Lemmon)
19:23:48.07 -03:38:59.5 14.2mag C/2023 R1 (PANSTARRS)
21:40:34.48 +85:07:17.5 17.8mag C/2023 X2 (Lemmon)
06:15:34.68 +63:32:53.8 17.1mag C/2024 A1 (ATLAS)
05:00:24.14 +16:12:43.6 10.7mag C/2024 E1 (Wierzchos)
16:22:51.91 +05:25:59.0 17.4mag C/2024 G6 (ATLAS)
20:19:00.24 +13:42:58.0 14.7mag C/2024 J3 (ATLAS)
03:21:12.15 -23:17:14.4 16.4mag C/2024 T5 (ATLAS)
05:11:52.06 +46:46:23.1 17.7mag C/2025 J1 (Borisov)
14:03:00.55 +41:06:58.8 14.9mag C/2025 L1 (ATLAS)
03:16:15.89 -25:19:33.2 17.8mag C/2025 Q3 (ATLAS)
23:06:44.89 +19:42:38.4 9.4mag C/2025 R3 (PANSTARRS)
12:56:39.33 +02:39:00.0 17.5mag C/2025 Y1 (ATLAS)
02:30:00.26 +03:30:10.3 10.9mag C/2026 A1 (MAPS)
23:42:44.16 +36:05:29.7 14.4mag C/2026 B2 (Sun-Gao)
18:31:34.52 -10:01:25.0 12.2mag 10P/Tempel
15:08:00.89 +03:46:33.0 13.5mag 24P/Schaumasse
11:04:28.73 -01:43:17.6 15.7mag 29P/Schwassmann-Wachmann
17:58:49.28 -09:49:57.5 17.8mag 40P/Vaisala
10:38:06.62 -04:35:09.6 16.8mag 43P/Wolf-Harrington
01:39:40.38 +16:29:16.9 17.2mag 47P/Ashbrook-Jackson
07:00:13.38 +38:15:05.3 17.0mag 63P/Wild
23:21:32.79 -12:09:34.2 15.7mag 65P/Gunn
03:47:53.37 +19:12:12.7 15.9mag 76P/West-Kohoutek-Ikemura
00:52:45.24 +07:04:40.8 14.4mag 78P/Gehrels
22:45:06.61 -11:06:34.3 14.6mag 88P/Howell
01:54:05.02 +19:03:42.0 15.1mag 93P/Lovas
04:44:01.08 +31:57:52.9 16.3mag 123P/West-Hartley
08:21:51.43 +41:03:06.4 16.2mag 124P/Mrkos
02:24:15.70 +13:42:49.4 16.4mag 128P/Shoemaker-Holt
02:36:08.30 +13:46:05.3 17.5mag 131P/Mueller
00:55:56.62 +11:08:21.7 10.9mag 141P/Machholz
01:05:35.03 +02:41:05.2 11.0mag 141P-A/Machholz
23:53:52.59 -01:09:18.1 13.5mag 141P-D/Machholz
01:35:17.71 +04:24:19.7 17.9mag 141P-I/Machholz
00:46:10.04 -04:26:41.4 15.2mag 162P/SidingSpring
10:29:51.27 +31:15:08.3 17.9mag 164P/Christensen
06:25:44.39 +24:25:18.8 17.9mag 198P/ODAS
15:01:46.27 -00:42:34.5 17.5mag 210P/Christensen
21:21:28.88 -12:51:27.4 17.5mag 218P/LINEAR
17:14:36.28 -14:37:18.4 16.2mag 235P/LINEAR
05:22:00.65 +34:13:28.6 16.7mag 240P/NEAT
07:35:48.08 -05:49:02.2 17.7mag 242P/Spahr
15:44:44.70 +06:35:38.7 17.5mag 391P/Kowalski
07:32:07.04 +21:20:24.5 17.6mag 450P/LONEOS
05:27:28.96 +45:22:29.6 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 23:24 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 9 23:24 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:18:48.927 -23:32:12.08 AT 2026ike 2026-02-12.51 20.2
08:47:41.490 -21:46:40.10 AT 2026ikd 2026-03-28.41 19.49
08:34:30.248 -07:09:24.85 AT 2026ikc 2026-03-29.44 19.28
13:21:25.078 +79:09:18.53 AT 2026ikb 2026-03-25.43 20.7322
09:05:18.124 -19:48:21.41 AT 2026ika 2026-03-09.36 20.58
08:38:25.468 +06:11:03.79 AT 2026ijz 2026-03-09.32 21.99
08:00:34.010 +04:48:18.04 AT 2026ijy 2026-03-09.31 21.07
09:02:07.082 +07:27:03.87 AT 2026ijx 2026-02-17.43 21.29
10:37:20.784 +30:59:50.95 AT 2026ijw 2026-03-10.33 20.2
16:00:37.915 +06:38:30.61 AT 2026ijv 2026-03-28.57 20.5
13:51:30.137 +25:53:04.17 AT 2026iju 2026-03-28.41 20.07
12:52:01.341 -19:06:48.80 AT 2026ijt 2026-01-28.59 20.22
11:38:25.995 -11:34:40.48 AT 2026ijs 2026-01-16.56 21.1
07:12:41.661 +56:25:20.59 AT 2026ijr 2026-01-19.40 20.76
09:34:48.813 +06:57:40.76 AT 2026ijq 2026-01-26.43 21.57
10:49:59.384 +25:17:19.22 AT 2026ijp 2026-04-04.17 19.836
08:20:22.449 +03:44:22.06 AT 2026ijo 2026-04-02.18 19.8276
06:41:34.987 -19:08:36.17 AT 2026ijn 2026-02-05.26 20.38
12:35:13.975 +41:45:24.96 AT 2026ijm 2026-04-02.31 19.9925
13:25:11.624 +08:21:44.99 AT 2026ijl 2026-03-27.40 20.8103
-rw-r--r-- 1 apache apache 30K Apr 9 23:24 tns_transients_list.txt
