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-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6585,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 13.73CV 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
target,2461140.6585,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
Gaia DR3 3114484440798411904,2461140.6585,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114484440798411904 20260410.1585 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
Gaia DR3 3108701280217431680,2461140.6585,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108701280217431680 20260410.1585 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 J106.5222-01.7271,2461140.6585,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5222-01.7271 20260410.1585 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5595-04.6017,2461140.6585,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5595-04.6017 20260410.1585 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 J104.0781-01.8195,2461140.6585,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.0781-01.8195 20260410.1585 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 J104.1174-02.9061,2461140.6585,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.1174-02.9061 20260410.1585 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6585,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
ATO J104.8482-01.3642,2461140.6585,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8482-01.3642 20260410.1585 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
Gaia DR3 3102494433997697024,2461140.6585,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102494433997697024 20260410.1585 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
NSVS 12532276,2461140.6585,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 12532276 20260410.1585 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,2461140.6585,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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,2461140.6585,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3125529340040233216,2461140.6585,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125529340040233216 20260410.1585 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
ASASSN-V J064630.95+010809.2,2461140.6585,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064630.95+010809.2 20260410.1585 13.30CV 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
target,2461140.6585,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
Gaia DR3 3109210942517493504,2461140.6585,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109210942517493504 20260410.1585 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
ATO J101.7538-03.8016,2461140.6585,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.7538-03.8016 20260410.1585 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
Gaia DR3 3107772540789231360,2461140.6585,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107772540789231360 20260410.1585 12.97CV 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
target,2461140.6585,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
target,2461140.6585,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
ATO J104.6016-03.2501,2461140.6585,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6016-03.2501 20260410.1585 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
ASASSN-V J063615.20+010007.8,2461140.6585,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J063615.20+010007.8 20260410.1585 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3113790030488561920,2461140.6585,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113790030488561920 20260410.1585 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,2461140.6585,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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,2461140.6585,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3109005952316009984,2461140.6585,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109005952316009984 20260410.1585 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
target,2461140.6585,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
ATO J105.0500-03.7984,2461140.6585,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0500-03.7984 20260410.1585 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 3101696433373426816,2461140.6585,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101696433373426816 20260410.1585 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,2461140.6585,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 J104.6569+01.3693,2461140.6585,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6569+01.3693 20260410.1585 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 3112377913960540288,2461140.6585,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112377913960540288 20260410.1585 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
ATO J103.6002-04.1912,2461140.6585,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6002-04.1912 20260410.1585 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 J107.2021-03.7245,2461140.6585,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.2021-03.7245 20260410.1585 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
ATO J107.4191-04.3825,2461140.6585,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4191-04.3825 20260410.1585 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3114694099624336256,2461140.6585,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114694099624336256 20260410.1585 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
Gaia DR3 3101503262931004032,2461140.6585,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101503262931004032 20260410.1585 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 3107459557930729984,2461140.6585,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107459557930729984 20260410.1585 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 3101503262931006720,2461140.6585,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101503262931006720 20260410.1585 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 3101475259743515520,2461140.6585,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101475259743515520 20260410.1585 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 J107.0282-02.1738,2461140.6585,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0282-02.1738 20260410.1585 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
target,2461140.6585,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3102372667384237952,2461140.6585,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102372667384237952 20260410.1585 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 3053304074782543488,2461140.6585,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053304074782543488 20260410.1585 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0385 Mon,2461140.6585,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0385 Mon 20260410.1585 12.51CV 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
target,2461140.6585,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 J105.0552-01.8046,2461140.6585,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0552-01.8046 20260410.1585 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
Gaia DR3 3101503056772630528,2461140.6585,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101503056772630528 20260410.1585 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 3109235166132304128,2461140.6585,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109235166132304128 20260410.1585 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 J101.7813-01.8578,2461140.6585,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.7813-01.8578 20260410.1585 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7797-03.0546,2461140.6585,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260410.1585 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
target,2461140.6585,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 12.18CV 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 3109471389332247552,2461140.6585,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109471389332247552 20260410.1585 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
ATO J104.7305-03.0153,2461140.6585,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7305-03.0153 20260410.1585 12.18CV 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 3107032775621691520,2461140.6585,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107032775621691520 20260410.1585 12.14CV 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 J106.4621-02.0972,2461140.6585,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.4621-02.0972 20260410.1585 11.93CV 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
ASAS J070940-0536.0,2461140.6585,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J070940-0536.0 20260410.1585 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 3125658296436103552,2461140.6585,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125658296436103552 20260410.1585 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3071-00.0429,2461140.6585,10.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3071-00.0429 20260410.1585 10.55CV 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 3113144097467624576,2461140.6585,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113144097467624576 20260410.1585 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.5593+02.0025,2461140.6585,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5593+02.0025 20260410.1585 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112051973180962048,2461140.6585,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112051973180962048 20260410.1585 12.13CV 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 J104.2896-03.9733,2461140.6585,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2896-03.9733 20260410.1585 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 J105.0068-05.1648,2461140.6585,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0068-05.1648 20260410.1585 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065448.56+002321.1,2461140.6585,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065448.56+002321.1 20260410.1585 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113847342532829952,2461140.6585,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113847342532829952 20260410.1585 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 J100.9536+01.2405,2461140.6585,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9536+01.2405 20260410.1585 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
Gaia DR3 3105621277567743360,2461140.6585,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105621277567743360 20260410.1585 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
ATO J100.6619-02.2718,2461140.6585,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6619-02.2718 20260410.1585 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 J104.6490-04.3421,2461140.6585,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6490-04.3421 20260410.1585 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461140.6585,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 J106.0676-03.0161,2461140.6585,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0676-03.0161 20260410.1585 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
Gaia DR3 3107281540128223104,2461140.6585,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107281540128223104 20260410.1585 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 3101061637209619328,2461140.6585,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101061637209619328 20260410.1585 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
MGAB-V1900,2461140.6585,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MGAB-V1900 20260410.1585 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
target,2461140.6585,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 J100.1094-03.5204,2461140.6585,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.1094-03.5204 20260410.1585 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
Gaia DR3 3114279450600387456,2461140.6585,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114279450600387456 20260410.1585 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
Gaia DR3 3105302487915881984,2461140.6585,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105302487915881984 20260410.1585 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
Gaia DR3 3105947282767695360,2461140.6585,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105947282767695360 20260410.1585 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
Gaia DR3 3105921684761121152,2461140.6585,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105921684761121152 20260410.1585 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
Gaia DR3 3109656416522583808,2461140.6585,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109656416522583808 20260410.1585 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
target,2461140.6585,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3113967635975814912,2461140.6585,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113967635975814912 20260410.1585 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
Gaia DR3 3125637852391270784,2461140.6585,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125637852391270784 20260410.1585 12.95CV 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
target,2461140.6585,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126002336198034048,2461140.6585,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126002336198034048 20260410.1585 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 3113534462753024768,2461140.6585,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113534462753024768 20260410.1585 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 3125762818759969664,2461140.6585,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125762818759969664 20260410.1585 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 3100477590376004224,2461140.6585,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100477590376004224 20260410.1585 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
ATO J107.1574+00.2897,2461140.6585,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1574+00.2897 20260410.1585 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
CoRoT 102806577,2461140.6585,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102806577 20260410.1585 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
target,2461140.6585,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3113913996125565440,2461140.6585,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260410.1585 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
Gaia DR3 3101401729901835904,2461140.6585,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101401729901835904 20260410.1585 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
GDS_J0656565-052329,2461140.6585,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0656565-052329 20260410.1585 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 3106128697885405184,2461140.6585,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106128697885405184 20260410.1585 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 3114460526421262848,2461140.6585,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114460526421262848 20260410.1585 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 J102.9043-01.6544,2461140.6585,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9043-01.6544 20260410.1585 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 3105302831513609216,2461140.6585,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105302831513609216 20260410.1585 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
ATO J103.0736-03.3663,2461140.6585,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0736-03.3663 20260410.1585 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,2461140.6585,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
Gaia DR3 3108863080225629056,2461140.6585,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108863080225629056 20260410.1585 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,2461140.6585,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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,2461140.6585,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3107527727657145984,2461140.6585,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107527727657145984 20260410.1585 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
target,2461140.6585,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
target,2461140.6585,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 3113700076693885568,2461140.6585,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113700076693885568 20260410.1585 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 3113219246514568576,2461140.6585,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260410.1585 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
Gaia DR3 3112578162515589760,2461140.6585,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112578162515589760 20260410.1585 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
ATO J101.9913-01.3476,2461140.6585,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9913-01.3476 20260410.1585 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
ATO J104.7479+00.9409,2461140.6585,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7479+00.9409 20260410.1585 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
Gaia DR3 3108875037416696192,2461140.6585,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108875037416696192 20260410.1585 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
Gaia DR3 3125885581805542656,2461140.6585,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125885581805542656 20260410.1585 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
Gaia DR3 3105901103278785152,2461140.6585,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105901103278785152 20260410.1585 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,2461140.6585,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
ATO J103.9614-02.2114,2461140.6585,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9614-02.2114 20260410.1585 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
Gaia DR3 3125767491683972224,2461140.6585,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125767491683972224 20260410.1585 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
ATO J104.9413-02.3695,2461140.6585,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9413-02.3695 20260410.1585 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
Gaia DR3 3113254705765810944,2461140.6585,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113254705765810944 20260410.1585 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.6375-01.8671,2461140.6585,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.6375-01.8671 20260410.1585 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 3106021564222428032,2461140.6585,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106021564222428032 20260410.1585 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.6585,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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 J103.2459-03.9011,2461140.6585,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.2459-03.9011 20260410.1585 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,2461140.6585,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
Gaia DR3 3112223325200684160,2461140.6585,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112223325200684160 20260410.1585 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
TX Mon,2461140.6585,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TX Mon 20260410.1585 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101904546012204032,2461140.6585,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101904546012204032 20260410.1585 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
Mean magnitude and position on the discovery images:
2026 04 10.1585 2461140.6585 13.62 07:02:38.31 +01:10:27.1
213.16334 3.02736 galactic Mon Second-epoch detections are separated by 3.7" and 7.6 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 3114610674178271616 | 07:02:38.31 +01:10:27.1 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.353+/-0.045 (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 3114610674178271616,2461140.6585,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3114610674178271616 20260410.1585 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,2461140.6585,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 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
ATO J103.8630-04.5748,2461140.6585,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8630-04.5748 20260410.1585 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
Gaia DR3 3119353181365762048,2461140.6585,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119353181365762048 20260410.1585 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
ATO J104.6381-01.6369,2461140.6585,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260410.1585 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
Gaia DR3 3106335238572484096,2461140.6585,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106335238572484096 20260410.1585 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
Gaia DR3 3112632309164197888,2461140.6585,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112632309164197888 20260410.1585 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.0072-01.5341,2461140.6585,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.0072-01.5341 20260410.1585 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
ATO J102.9282-03.6451,2461140.6585,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9282-03.6451 20260410.1585 13.67CV 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
target,2461140.6585,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.1327-06.2379,2461140.6585,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.1327-06.2379 20260410.1585 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,2461140.6585,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.1585 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461140.65884366 10.04.2026 03:48:34.092 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
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: 9 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): 30436
Objects passed selection criteria: 30310
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 23780.2
Average stars matched: 21567 (90.6929 %)
Memory usage VmPeak: 131292 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 22:51:18 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461140.65884366 10.04.2026 03:48:34.092 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 390
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 240 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): 224146
Objects passed selection criteria: 223443
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 181803
Average stars matched: 165627 (91.1025 %)
Memory usage VmPeak: 1976988 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 22:57:09 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461140.65825289
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:32.413 -01:59:29.19
Angular distance between the image centers 0.0464 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 06:51:34.066 -02:00:07.26
Angular distance between the image centers 0.0376 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 06:51:32.413 -01:59:29.19
Second-epoch second image center 06:51:34.066 -02:00:07.26
Angular distance between the image centers 0.01262 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.iBOX3DLAad
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.00B3QFbOmQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits &> /tmp/tmp.HW6d4MwWtW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits &> /tmp/tmp.NdHCIwDKPK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
2.6 pix fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.6 mag. fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
14.5 mag. fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (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.iBOX3DLAad (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
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-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.00B3QFbOmQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
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.HW6d4MwWtW (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-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2387, passed=25748
Got 25748 stars (including 23347 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 25748 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 25296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 25294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 25294 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NdHCIwDKPK (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-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2412, passed=25470
Got 25470 stars (including 23035 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 25470 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 24868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 24871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 24871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 928 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58135.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51879_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 51879_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:07.49 -01:28:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 2.243 3106909213700454528 099.53163508451 -01.46839862892 11.0128 10.8637 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 51881_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 51881_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:04:59.46 -05:12:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 1.275 3101435952202000768 106.24765874339 -05.20259220735 10.6954 10.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53794_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 53794_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:13.66 -02:21:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54953_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 54953_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:37.29 -03:49:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55800_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 55800_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:49.55 +00:28:06.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57803_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 57803_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:45.33 +00:41:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58135_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 58135_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:58.41 +00:32:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 2.617 3113027519173665152 105.74308942653 +00.53505361358 12.0753 11.6712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:32.413 -01:59:29.19
Angular distance between the image centers 0.0464 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 06:51:34.066 -02:00:07.26
Angular distance between the image centers 0.0376 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 06:51:32.413 -01:59:29.19
Second-epoch second image center 06:51:34.066 -02:00:07.26
Angular distance between the image centers 0.01262 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.qUHOzWpAa0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.av2x2k5mK4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits &> /tmp/tmp.xWMC8Dil6d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits &> /tmp/tmp.5Pm4lYFzel
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 309 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.3 pix fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
13.9 mag. fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.qUHOzWpAa0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
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-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.av2x2k5mK4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
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.xWMC8Dil6d (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-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=66, blended=26421, passed=184281
Got 184281 stars (including 157689 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 184281 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 181459 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 181455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 181456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.5Pm4lYFzel (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-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=26418, passed=184948
Got 184948 stars (including 158341 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat
util/solve_plate_with_UCAC5 got 184948 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 181583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 181584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 181585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 928 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-47-43_20.00sec_-5.00C_LIGHT_0020.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Mon-02-Q2b1x1_224924_TTUQ2b1x1_783_lf4brXft/wcs_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out283563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302026.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out305105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310524.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out311605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311675.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out311938.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out312931.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out313530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314269.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out314625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315226.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out315285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316672.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out320910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out283542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283620.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283702.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out287148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315736.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323756.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 172s
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: 96s
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Considering the candidate 283542_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283542_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283550_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283550_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283563_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283563_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:22.70 +01:39:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.705 3126700392941715968 099.34465066702 +01.66253109780 14.3637 13.7104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283570_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283570_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:47.85 +00:54:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.643 3125793811243900160 100.69918572088 +00.91358921301 14.7339 14.3129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283575_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283575_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:34.70 -05:36:35.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 283577_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283577_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283581_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283581_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283588_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283588_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:04:30.11 -02:50:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.503 3108755641625156352 106.12479812681 -02.83504894910 14.5004 14.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283610_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283610_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283611_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283611_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:11.90 +00:14:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.387 3125505704838714496 101.29941187509 +00.23685264125 14.4374 13.9985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283615_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283615_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 283620_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283620_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283623_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283623_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:22.43 +00:33:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.949 3113590086878300544 102.84295080789 +00.56088917339 14.3448 13.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283643_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283643_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:57:58.54 -02:26:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.286 3108974753674060160 104.49397748305 -02.44468853161 14.4713 13.9570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283645_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283645_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283659_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283659_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:26.47 -01:58:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 4.777 3109201008252280320 106.85906758044 -01.97104186546 14.4383 13.5709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283663_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283663_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:25.32 -02:10:12.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 283681_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283681_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283691_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283691_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283692_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283692_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283699_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283699_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:09.29 +00:44:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.525 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283702_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283702_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283720_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283720_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:48.80 +00:23:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.708 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 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 283728_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283728_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:37.51 -01:11:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.011 3112186010523071488 104.90629502068 -01.18861419962 14.2398 13.4815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283738_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283738_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283741_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283741_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283744_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283744_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:19.82 -00:56:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.595 3112568954105823744 105.33361949851 -00.94546764897 14.2680 13.7804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283754_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283754_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283755_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283755_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 283756_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283756_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283758_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283758_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:39:49.01 +01:08:52.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 283764_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283764_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283768_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283768_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283771_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283771_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283778_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283778_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283780_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283780_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:51.00 -05:12:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.380 3101581706207521280 104.96246888320 -05.20313260263 13.9922 13.4966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283782_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283782_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:32.62 -04:52:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.945 3059428423269301248 107.13498037393 -04.87093591462 13.8481 13.1876 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#
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Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283803_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:15.41 -00:32:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.985 3112636294895145472 105.31420401818 -00.55077355714 14.1181 13.6386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283805_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283805_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283806_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283806_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:01.08 +00:39:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.808 3113078680823551744 105.50499158530 +00.65039666052 14.2419 13.4343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283811_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283811_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:58.77 +00:11:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.315 3112759547573659008 106.49478838253 +00.18855727320 14.1112 13.5262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283812_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283812_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283814_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283814_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283815_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283815_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283817_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283817_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:48.04 -01:23:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.772 3112343726021758336 102.94940029937 -01.39027097196 13.8590 13.0180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283819_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283819_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283821_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283821_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:53.32 +01:01:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.386 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283837_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283837_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 283843_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283843_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:51.86 +01:20:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.230 3115367211199527296 105.46601850960 +01.33474391831 14.0347 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283847_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283847_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283853_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283853_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:52.34 -00:44:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.158 3109635113484885248 107.21776257479 -00.74292765116 13.7584 13.3194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283855_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283855_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:45.04 -03:41:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.996 3107703821317850368 107.43704622586 -03.69891737982 13.8124 13.3638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283863_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283863_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:29.27 -03:35:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.483 3102754163561342208 103.62189494822 -03.59079608507 13.8389 12.9507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283869_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283869_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283871_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283871_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283872_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283872_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:06.96 -04:44:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.294 3103740803447657984 100.77900589386 -04.73877605323 13.9479 13.3967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283873_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283873_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:56.93 +00:43:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.961 3125594799639377024 100.73738555000 +00.73187374331 13.4606 12.4772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283876_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283876_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:57:47.24 -05:04:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.701 3101596167357260288 104.44675208096 -05.07321561344 13.7730 13.4522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283879_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283879_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283881_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283881_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:37.97 +00:05:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.522 3119509685677083136 100.90815124971 +00.09182959907 13.7914 13.3091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283893_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283893_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283899_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283899_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283905_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283905_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283908_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283908_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:19.36 -01:29:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.620 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283923_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283923_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283928_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283928_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:52.41 -02:39:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.150 3105924708418098176 102.46828545603 -02.66550711271 13.6843 13.1955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283934_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283934_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:37.44 -02:21:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.696 3106690204730551936 099.65602265592 -02.35585984284 13.2484 12.1574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283946_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:04.39 -05:53:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.490 3101108259073557760 103.01829861414 -05.88727505251 13.5348 13.0509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283948_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283948_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283957_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283957_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283958_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:25.62 +02:12:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.925 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283960_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283960_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:18.32 -05:27:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.223 3100667290492598144 101.07632058798 -05.45614390659 13.5828 13.1018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283962_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283962_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283963_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:43.49 +01:59:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.569 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283973_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283973_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283976_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283976_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:46.84 -00:33:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.800 3113199352226204672 102.44499550161 -00.55439773710 13.4120 12.8854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283977_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283977_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:54.57 +01:24:50.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283985_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 283985_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:58.31 -00:59:20.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 283989_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283989_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 283997_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 283997_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284001_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284001_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:12.59 +00:51:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.557 3125567930324132096 101.55227975245 +00.85185603769 13.4133 12.9328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284005_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284005_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:16.30 +01:31:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 3.224 3113937227607500032 104.81750267812 +01.51665013383 13.1344 12.7039 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#
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Considering the candidate 284009_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284009_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284010_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284010_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284012_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284012_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284022_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284022_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284024_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284024_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284029_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284029_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284032_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284032_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:42.31 -03:09:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.661 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284033_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284033_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:08.21 -05:53:00.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 284035_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284035_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284036_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284036_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:02.41 +01:07:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284042_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284042_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284045_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284045_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:18.43 -01:42:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.790 3109224617692615680 107.32664531728 -01.70983647051 12.2567 11.3087 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 284046_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284046_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:05:06.81 -05:11:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 2.042 3101436089640924288 106.27801245259 -05.18913182412 12.7221 11.8027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284052_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284052_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:13.92 -05:00:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284065_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284065_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:35.61 +01:46:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284068_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284068_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:11.74 -01:33:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284070_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284070_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284071_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284071_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:26.03 -01:50:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284073_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 284073_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 284077_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284077_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:07:49.52 -05:43:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284078_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 284078_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:59.02 -04:51:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 0.529 3102224366453166976 101.49580560879 -04.86373564501 11.8140 11.5763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 287079_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 287079_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:40.16 -00:32:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 287148_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 287148_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 288959_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 288959_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:37.21 +00:26:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289590_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 289590_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:15.60 +01:46:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289703_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 289703_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 289736_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 289736_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:51:39.70 +00:25:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289965_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 289965_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:37.71 +00:43:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291129_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 291129_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:04:10.70 -03:14:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291182_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 291182_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:30.50 -01:04:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292121_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 292121_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:41.56 -00:33:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 293578_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 293578_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:36:41.07 -05:13:21.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 293754_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 293754_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 296699_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 296699_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:52.67 -01:19:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 298448_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 298448_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:44.43 -00:31:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 299166_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 299166_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:16.35 -04:45:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299282_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 299282_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:39.57 -04:37:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299298_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 299298_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:00.21 -00:03:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299431_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299431_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 299995_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 299995_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 300801_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 300801_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:34:15.00 -05:19:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.062 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300869_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 300869_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:54.24 +00:00:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.838 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300911_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 300911_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:06.98 -01:31:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.700 3118812874479474048 098.77860290306 -01.52424273167 13.1457 12.5678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301450_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 301450_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:04.76 -01:02:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.313 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301494_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 301494_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:03.43 -02:29:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.296 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 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#
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Considering the candidate 301722_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 301722_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 302026_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 302026_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:13.64 +01:34:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.161 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303211_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 303211_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 303318_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 303318_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:43:50.66 +01:35:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303501_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 303501_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:03.29 -06:07:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303895_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 303895_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:22.45 -03:06:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304524_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 304524_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:17.46 -04:25:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.547 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304935_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 304935_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:26.07 -06:06:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305105_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 305105_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:06.13 -00:02:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.517 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305395_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 305395_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:07.37 -01:52:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305876_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 305876_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:18.53 -00:51:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.714 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305908_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 305908_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 306759_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 306759_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:23.33 -01:37:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.874 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306762_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 306762_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:14.72 -02:18:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.310 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306853_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 306853_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 307245_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 307245_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 307446_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 307446_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 307979_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 307979_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:59.85 -02:44:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 5.620 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308255_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 308255_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:55.08 -02:23:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 2.390 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308365_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 308365_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 308478_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 308478_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 308714_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 308714_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 308771_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 308771_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 308943_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 308943_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:43.13 +02:11:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309523_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 309523_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 309632_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 309632_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 309767_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 309767_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:12.49 -05:08:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.586 3100657291808314112 101.55197132706 -05.14813242199 13.6082 12.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309816_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 309816_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:26.82 -00:55:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.883 3112570461635443584 105.36207810215 -00.92448145232 13.7792 12.9935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309905_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 309905_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 309984_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 309984_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:36:19.10 +00:01:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.658 3119670321748998144 099.07841400793 +00.02333476458 13.6081 12.5499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310171_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 310171_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 310186_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 310186_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:10.30 -05:37:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 2.958 3100436324330257664 101.79278991116 -05.62100639477 13.7323 13.3078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310335_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 310335_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 310524_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 310524_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:13.98 -00:06:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.657 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310610_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 310610_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 310771_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 310771_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:33.36 +01:51:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311043_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 311043_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:20.36 -05:15:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.337 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311309_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 311309_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:20.49 -00:31:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311478_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 311478_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 311605_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 311605_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:30.61 +00:57:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.194 3125654791743165184 102.12743384694 +00.96221421685 13.6988 13.2550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311675_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 311675_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:26.04 -01:49:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.770 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311692_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 311692_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 311740_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 311740_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 311778_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 311778_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 311868_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 311868_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:42:29.63 -04:08:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.261 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311894_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 311894_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 311938_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 311938_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:57.08 -02:34:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.111 3106665332578815488 098.98842000814 -02.57393459680 13.6156 12.7486 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 311990_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 311990_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 312116_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 312116_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 312137_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 312137_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 312385_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312385_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:22.96 -02:46:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.968 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312423_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 312423_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 312516_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312516_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:40:05.29 -04:41:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.897 3103780042268573568 100.02241043894 -04.69454432899 13.8502 13.0386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312544_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 312544_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 312617_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 312617_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 312655_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312655_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:00:53.47 +02:12:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.985 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312696_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312696_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:58:50.11 -04:41:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.640 3101679906339288704 104.70859973578 -04.68774296413 13.8134 13.3106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312883_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312883_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:39:24.93 +00:07:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.662 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312931_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312931_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:20.97 -03:11:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.951 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312972_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 312972_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:21.08 -05:34:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.990 3101891734129376896 103.08775253888 -05.57718780004 13.3163 12.2056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313106_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313106_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 313190_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313190_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313309_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313309_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313406_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313406_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313485_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313485_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313496_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313496_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 313530_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 313530_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:09.63 -05:17:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 4.585 3100639871420927872 101.78975441255 -05.28971896782 13.7735 12.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313741_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 313741_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:59.29 -05:34:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.173 3101926196945967232 102.24738757339 -05.57946786713 13.8133 12.9787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313777_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 313777_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:53.11 +01:49:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.753 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313839_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 313839_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 314269_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314269_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:47.06 -00:07:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.935 3113468973092058240 101.69553406151 -00.13282456161 14.0572 13.1422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314312_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314312_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:55:58.72 -01:35:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 2.689 3112099187762874112 103.99454201873 -01.60068098726 13.8572 13.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314423_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314423_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:59.56 -01:03:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.528 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314572_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314572_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:41:20.99 -01:43:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.374 3106831942950099584 100.33652100745 -01.72233248144 13.6881 12.6456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314625_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314625_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:41.43 -00:33:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.925 3112503842401083904 103.42233870049 -00.56409058978 14.0403 13.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314681_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314681_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:34:30.94 +01:34:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.266 3120870095095731712 098.62977890512 +01.56941165889 14.0172 13.2389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314827_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 314827_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:39:08.59 -03:48:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.781 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315065_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 315065_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:14.23 +00:45:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.932 3125565078465888768 101.55954576647 +00.75816110703 13.9059 12.9956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315093_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315093_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315164_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315164_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315198_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 315198_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:36:32.39 -03:35:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.898 3104844850559457792 099.13443358317 -03.59975014338 14.0155 13.4377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315217_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315217_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315226_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 315226_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:56.42 -04:43:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.458 3102055458280756864 103.48505444976 -04.73232095785 14.0018 13.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315259_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 315259_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:04.42 -01:43:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.448 3109233104548149120 107.01874958326 -01.72878742697 13.9560 13.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315285_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 315285_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:06:14.83 -04:55:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.617 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315458_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315458_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315525_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315525_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315607_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315607_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315629_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315629_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315736_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315736_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 315784_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315784_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315788_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 315788_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:34.60 +00:32:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.828 3113580985840503296 103.14371971951 +00.54139619495 14.0748 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315874_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 315874_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 316091_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 316091_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316155_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 316155_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316170_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 316170_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:33.73 -00:26:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.563 3107451723910491520 101.39020146722 -00.43924863840 14.0394 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316370_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 316370_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:52.46 +01:12:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.705 3120620024919006848 099.71870063274 +01.20611895865 14.1237 13.6672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316520_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 316520_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:14.59 -03:39:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.317 3105452708691209216 101.81087051013 -03.65148798860 13.4646 12.2211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316672_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 316672_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:10.41 -00:43:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.624 3119206774519517696 098.79348040669 -00.72377880410 14.0197 13.4537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316759_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 316759_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:35.47 +01:49:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.319 3126715957902670336 099.39769433910 +01.82061329003 14.0033 13.4872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316805_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 316805_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:04.09 +01:58:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.146 3126360472050420992 101.76704300021 +01.97593177349 13.9878 13.4960 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#
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Considering the candidate 317166_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 317166_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317197_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 317197_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317235_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 317235_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:01.06 -03:51:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.745 3102403384990262912 102.50427467152 -03.86454680347 13.9866 13.4513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317436_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 317436_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:44:57.53 -02:51:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.664 3105761838958624896 101.23984910248 -02.86210694641 14.0439 13.5422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317471_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 317471_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 317550_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 317550_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:13.92 -05:27:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.233 3100630594291784192 101.55802271223 -05.45858847386 14.0725 13.1686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317570_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 317570_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:27.81 -05:57:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.150 3101095172312498048 103.11590743628 -05.95317978863 14.0687 13.5555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317654_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 317654_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 317761_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 317761_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 317797_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 317797_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 317913_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 317913_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 317966_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 317966_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:38.05 -00:17:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.952 3119433956814456704 099.65819127034 -00.29763616830 14.2367 13.6075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318021_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 318021_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 318481_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 318481_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 318661_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 318661_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 318955_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 318955_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:57.51 -02:12:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.374 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318983_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 318983_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 319228_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 319228_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:45.26 +01:25:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.145 3114076418906304512 103.43838803221 +01.42863147043 14.0414 13.1455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319437_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 319437_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 319500_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 319500_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 319506_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 319506_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:58:25.99 -05:48:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.216 3100992264898211584 104.60868983330 -05.80991184590 14.0487 13.5345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319544_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 319544_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:07.99 -00:50:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.499 3112396262060776064 103.28294642765 -00.84221327009 14.2623 13.7125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319705_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 319705_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:38:53.38 -00:49:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.419 3119330641377186688 099.72224575617 -00.82187219144 14.2480 13.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319750_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 319750_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 319849_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 319849_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:47:27.47 -05:04:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.944 3102156029234873472 101.86457739760 -05.08341579408 14.1265 13.5611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319917_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 319917_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 319987_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 319987_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 320070_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 320070_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 320154_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 320154_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:53:47.83 +00:29:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.586 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320897_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 320897_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 320910_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 320910_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:35:16.60 -01:19:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.716 3118957632057909376 098.81878136857 -01.31878064928 14.3099 13.6904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321142_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 321142_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 321164_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 321164_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:49:38.79 +00:36:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.634 3113619949783427072 102.41144535065 +00.61020120759 13.8962 12.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321229_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 321229_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:39.61 -00:16:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.518 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321432_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 321432_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:05.48 +00:51:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.346 3113605484332811648 103.02252679260 +00.85637243039 14.3468 13.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321465_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 321465_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:46:39.51 -05:23:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.793 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321518_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 321518_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 321670_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 321670_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:18.14 -02:07:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.061 3106051805090685696 103.57553630608 -02.12473732458 14.3576 13.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321811_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 321811_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 321836_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 321836_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:03:36.10 -02:49:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.521 3108675136756949760 105.90026870374 -02.81891114047 14.3169 13.8437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321885_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 321885_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 321928_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 321928_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 322112_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 322112_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 322182_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 322182_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
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Considering the candidate 322196_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 322196_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:36.97 -01:46:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.380 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322279_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 322279_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322397_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 322397_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322694_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 322694_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322882_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 322882_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:57:45.90 -05:16:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.212 3101213919567915136 104.44138425122 -05.27926642880 14.5939 14.0088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322929_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 322929_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:39.56 +02:14:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.970 3126055215833740800 101.41533747424 +02.23645323046 14.4702 13.6105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323056_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323056_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:48:22.64 +01:01:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.906 3125668015943753984 102.09377189004 +01.01817011609 14.6347 14.0013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323136_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323136_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:45:47.99 -05:24:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.382 3100642276602853248 101.44966358979 -05.40758690969 13.9026 12.8468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323175_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 323175_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323186_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323186_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:59:12.05 -02:20:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.867 3108997293662134400 104.79962658383 -02.33451681197 14.6167 14.2326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323239_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 323239_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323304_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323304_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:47.30 +00:29:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.303 3113730072741558272 104.19687239559 +00.49405138811 14.6154 13.8350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323318_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323318_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:52:05.69 -01:36:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.643 3106285485671334784 103.02345645078 -01.60554724780 14.5023 13.6142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323512_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 323512_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323673_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323673_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:02:14.36 -05:25:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.038 3101348506667129088 105.55929233559 -05.43362203501 14.1968 13.1039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323701_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 323701_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323756_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
Preparing report for the candidate 323756_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323815_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323815_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:14.18 +00:13:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.208 3113369261132592512 103.55912634076 +00.23166545275 14.6377 13.8686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323902_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323902_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:56:56.87 +00:03:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.793 3112926742060801536 104.23687588539 +00.05258959081 14.3367 13.3942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323926_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323926_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:50:35.81 -00:13:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 4.787 3113245703512809600 102.64937841303 -00.23256876871 14.7616 14.1240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323953_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 323953_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:54:28.21 -00:30:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.271 3112510714348644608 103.61751004395 -00.51521349670 14.7702 14.1863 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324011_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 324011_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:01:54.12 -03:56:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.149 3101827343977192064 105.47546378355 -03.93567916949 14.7715 14.2350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:09:13.65 -02:21:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 07:08:45.31 +00:41:48.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-09_22-48-34_20.00sec_-4.90C_LIGHT_0021 did not pass the final checks
**** FOUND 06:37:53.18 -05:55:15.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 282s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:59:50.22 -01:50:12.6
06:50:18.38 -00:09:33.0
07:08:43.04 +01:24:45.4
06:59:51.88 -02:58:55.2
07:06:05.77 -01:43:45.8
07:02:14.60 -04:35:51.7
06:56:16.28 -01:49:31.2
06:56:26.15 -02:53:13.9
06:45:13.05 -00:39:26.7
06:59:25.27 -01:21:56.3
06:54:49.12 -04:18:06.6
06:52:01.28 +00:12:01.9
06:54:05.30 -01:51:49.2
06:50:00.15 -05:55:19.3
06:44:39.20 +00:25:38.3
06:46:31.25 +01:08:36.7
06:56:04.38 -01:30:01.3
07:09:26.85 -01:56:02.1
06:47:02.80 -03:47:40.7
07:04:59.57 -03:57:33.1
07:03:36.96 -00:12:37.0
06:53:04.48 -05:33:24.5
06:58:27.05 -03:14:41.7
06:36:15.18 +01:00:10.7
06:56:16.93 +00:50:18.8
06:45:26.97 -05:18:37.3
06:52:00.95 +01:29:16.3
06:59:42.15 -02:10:53.0
06:44:14.40 +00:14:37.9
07:00:12.21 -03:47:44.1
06:58:21.12 -04:33:28.4
07:05:05.72 -03:34:37.3
06:58:39.24 +01:21:58.9
06:53:41.51 -01:02:04.6
06:54:23.77 -04:11:38.3
07:08:48.79 -03:43:03.8
07:09:41.29 -04:22:46.2
07:07:06.92 +01:40:00.1
07:03:24.80 -05:00:17.1
06:46:00.26 -00:22:07.6
07:03:25.22 -05:00:42.3
07:05:45.28 -04:50:46.5
07:08:06.96 -02:10:36.2
07:02:17.29 -03:49:25.2
06:48:31.54 -04:05:33.1
07:07:51.42 -05:47:00.1
07:09:10.53 -05:50:47.5
06:46:13.89 +00:50:42.1
07:00:12.13 -01:48:12.9
07:03:26.97 -05:01:12.8
07:09:08.45 -01:41:28.8
06:47:07.68 -01:51:11.9
06:35:07.39 -03:03:05.0
07:08:11.94 -05:47:37.9
07:05:18.17 -01:23:00.4
06:58:57.09 -03:00:41.7
06:44:34.07 -01:35:28.6
07:05:50.97 -02:05:14.3
07:09:40.01 -05:35:35.3
06:47:12.95 +00:51:23.6
06:45:12.35 -00:01:52.9
06:50:14.49 -00:47:13.2
07:06:17.14 +02:00:14.9
06:58:06.51 -01:38:10.2
06:57:11.76 -03:58:12.3
07:00:01.25 -05:09:19.7
06:54:48.40 +00:23:18.2
06:59:33.51 +01:05:00.0
06:43:47.18 +01:14:20.6
06:42:33.20 -03:28:07.2
06:42:39.02 -02:16:08.3
06:58:35.62 -04:20:28.4
06:42:42.18 -01:42:37.2
07:04:16.73 -03:01:38.5
06:41:27.06 -01:19:04.7
06:55:24.49 -05:54:32.5
06:46:50.85 +01:18:08.8
07:01:10.13 -01:01:16.0
06:40:25.87 -03:31:15.1
07:08:49.43 +00:27:13.9
06:43:42.35 -04:26:31.3
06:54:41.89 -02:41:59.1
06:49:56.14 -02:40:56.0
07:08:59.17 -00:34:33.2
06:49:07.27 -01:40:17.9
06:53:54.81 +00:47:28.6
06:44:50.72 +01:05:45.8
07:05:38.61 +01:26:02.2
06:44:48.72 +01:46:40.8
06:47:41.04 +00:31:30.9
06:47:23.73 +01:25:43.4
06:42:30.94 -06:04:22.2
07:08:37.32 +00:17:23.6
06:46:10.29 -03:14:00.3
06:41:05.36 -05:41:10.7
06:57:35.69 +01:13:53.3
07:01:28.01 -05:15:08.4
06:56:58.48 -05:23:30.6
06:49:56.02 -02:17:05.3
07:09:21.64 +01:07:25.9
06:51:34.20 -01:39:24.1
06:43:36.94 -04:25:04.0
06:52:17.74 -03:21:56.6
06:49:24.59 -00:56:18.7
07:04:51.57 -02:12:05.5
06:48:56.92 -03:30:57.8
06:50:34.17 -02:44:35.6
07:09:33.72 -04:18:54.6
06:55:18.97 +01:47:06.4
06:52:27.33 -05:52:44.1
06:55:15.88 +00:20:56.6
06:50:41.42 -00:31:46.3
07:01:35.39 -00:48:25.8
06:47:59.52 -01:20:54.5
06:59:01.98 +00:56:29.5
07:03:45.94 -02:09:36.6
06:42:15.55 +01:14:36.6
06:50:48.55 -02:55:08.6
06:48:34.57 -03:13:30.7
06:55:50.72 -02:12:29.1
06:46:52.14 +01:30:31.7
06:59:46.60 -02:22:14.2
06:53:46.48 -00:31:17.1
06:46:32.53 -01:51:13.3
06:52:50.94 -02:20:52.1
06:51:30.59 +01:15:08.1
06:52:59.48 -03:53:54.2
06:48:04.22 -01:54:53.2
06:57:11.57 -01:07:45.5
06:50:52.35 -01:26:22.7
06:52:16.18 -05:20:42.3
07:02:38.31 +01:10:27.1
06:48:22.34 -00:23:14.0
06:55:27.97 -04:33:52.7
06:41:39.95 -00:36:38.7
06:58:34.65 -01:38:22.3
06:51:28.84 -01:28:30.1
07:01:45.53 -00:36:23.0
07:08:01.12 -01:31:56.5
06:51:44.83 -03:39:24.0
06:45:19.66 +01:14:09.0
06:52:33.58 -06:13:39.8
06:44:45.95 -02:03:56.6
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:59:50.22 -01:50:12.6
06:50:18.38 -00:09:33.0
07:08:43.04 +01:24:45.4
06:59:51.88 -02:58:55.2
07:06:05.77 -01:43:45.8
07:02:14.60 -04:35:51.7
06:56:16.28 -01:49:31.2
06:56:26.15 -02:53:13.9
06:45:13.05 -00:39:26.7
06:59:25.27 -01:21:56.3
06:54:49.12 -04:18:06.6
06:52:01.28 +00:12:01.9
06:54:05.30 -01:51:49.2
06:50:00.15 -05:55:19.3
06:44:39.20 +00:25:38.3
06:46:31.25 +01:08:36.7
06:56:04.38 -01:30:01.3
07:09:26.85 -01:56:02.1
06:47:02.80 -03:47:40.7
07:04:59.57 -03:57:33.1
07:03:36.96 -00:12:37.0
06:53:04.48 -05:33:24.5
06:58:27.05 -03:14:41.7
06:36:15.18 +01:00:10.7
06:56:16.93 +00:50:18.8
06:45:26.97 -05:18:37.3
06:52:00.95 +01:29:16.3
06:59:42.15 -02:10:53.0
06:44:14.40 +00:14:37.9
07:00:12.21 -03:47:44.1
06:58:21.12 -04:33:28.4
07:05:05.72 -03:34:37.3
06:58:39.24 +01:21:58.9
06:53:41.51 -01:02:04.6
06:54:23.77 -04:11:38.3
07:08:48.79 -03:43:03.8
07:09:41.29 -04:22:46.2
07:07:06.92 +01:40:00.1
07:03:24.80 -05:00:17.1
06:46:00.26 -00:22:07.6
07:03:25.22 -05:00:42.3
07:05:45.28 -04:50:46.5
07:08:06.96 -02:10:36.2
07:02:17.29 -03:49:25.2
06:48:31.54 -04:05:33.1
07:07:51.42 -05:47:00.1
07:09:10.53 -05:50:47.5
06:46:13.89 +00:50:42.1
07:00:12.13 -01:48:12.9
07:03:26.97 -05:01:12.8
07:09:08.45 -01:41:28.8
06:47:07.68 -01:51:11.9
06:35:07.39 -03:03:05.0
07:08:11.94 -05:47:37.9
07:05:18.17 -01:23:00.4
06:58:57.09 -03:00:41.7
06:44:34.07 -01:35:28.6
07:05:50.97 -02:05:14.3
07:09:40.01 -05:35:35.3
06:47:12.95 +00:51:23.6
06:45:12.35 -00:01:52.9
06:50:14.49 -00:47:13.2
07:06:17.14 +02:00:14.9
06:58:06.51 -01:38:10.2
06:57:11.76 -03:58:12.3
07:00:01.25 -05:09:19.7
06:54:48.40 +00:23:18.2
06:59:33.51 +01:05:00.0
06:43:47.18 +01:14:20.6
06:42:33.20 -03:28:07.2
06:42:39.02 -02:16:08.3
06:58:35.62 -04:20:28.4
06:42:42.18 -01:42:37.2
07:04:16.73 -03:01:38.5
06:41:27.06 -01:19:04.7
06:55:24.49 -05:54:32.5
06:46:50.85 +01:18:08.8
07:01:10.13 -01:01:16.0
06:40:25.87 -03:31:15.1
07:08:49.43 +00:27:13.9
06:43:42.35 -04:26:31.3
06:54:41.89 -02:41:59.1
06:49:56.14 -02:40:56.0
07:08:59.17 -00:34:33.2
06:49:07.27 -01:40:17.9
06:53:54.81 +00:47:28.6
06:44:50.72 +01:05:45.8
07:05:38.61 +01:26:02.2
06:44:48.72 +01:46:40.8
06:47:41.04 +00:31:30.9
06:47:23.73 +01:25:43.4
06:42:30.94 -06:04:22.2
07:08:37.32 +00:17:23.6
06:46:10.29 -03:14:00.3
06:41:05.36 -05:41:10.7
06:57:35.69 +01:13:53.3
07:01:28.01 -05:15:08.4
06:56:58.48 -05:23:30.6
06:49:56.02 -02:17:05.3
07:09:21.64 +01:07:25.9
06:51:34.20 -01:39:24.1
06:43:36.94 -04:25:04.0
06:52:17.74 -03:21:56.6
06:49:24.59 -00:56:18.7
07:04:51.57 -02:12:05.5
06:48:56.92 -03:30:57.8
06:50:34.17 -02:44:35.6
07:09:33.72 -04:18:54.6
06:55:18.97 +01:47:06.4
06:52:27.33 -05:52:44.1
06:55:15.88 +00:20:56.6
06:50:41.42 -00:31:46.3
07:01:35.39 -00:48:25.8
06:47:59.52 -01:20:54.5
06:59:01.98 +00:56:29.5
07:03:45.94 -02:09:36.6
06:42:15.55 +01:14:36.6
06:50:48.55 -02:55:08.6
06:48:34.57 -03:13:30.7
06:55:50.72 -02:12:29.1
06:46:52.14 +01:30:31.7
06:59:46.60 -02:22:14.2
06:53:46.48 -00:31:17.1
06:46:32.53 -01:51:13.3
06:52:50.94 -02:20:52.1
06:51:30.59 +01:15:08.1
06:52:59.48 -03:53:54.2
06:48:04.22 -01:54:53.2
06:57:11.57 -01:07:45.5
06:50:52.35 -01:26:22.7
06:52:16.18 -05:20:42.3
07:02:38.31 +01:10:27.1
06:48:22.34 -00:23:14.0
06:55:27.97 -04:33:52.7
06:41:39.95 -00:36:38.7
06:58:34.65 -01:38:22.3
06:51:28.84 -01:28:30.1
07:01:45.53 -00:36:23.0
07:08:01.12 -01:31:56.5
06:51:44.83 -03:39:24.0
06:45:19.66 +01:14:09.0
06:52:33.58 -06:13:39.8
06:44:45.95 -02:03:56.6
###################################################################################
06:59:50.22 -01:50:12.6 -- not an asteroid (will add it to exclusion list)
06:50:18.38 -00:09:33.0 -- not an asteroid (will add it to exclusion list)
07:08:43.04 +01:24:45.4 -- not an asteroid (will add it to exclusion list)
06:59:51.88 -02:58:55.2 -- not an asteroid (will add it to exclusion list)
07:06:05.77 -01:43:45.8 -- not an asteroid (will add it to exclusion list)
07:02:14.60 -04:35:51.7 -- not an asteroid (will add it to exclusion list)
06:56:16.28 -01:49:31.2 -- not an asteroid (will add it to exclusion list)
06:56:26.15 -02:53:13.9 -- not an asteroid (will add it to exclusion list)
06:45:13.05 -00:39:26.7 -- not an asteroid (will add it to exclusion list)
06:59:25.27 -01:21:56.3 -- not an asteroid (will add it to exclusion list)
06:54:49.12 -04:18:06.6 -- not an asteroid (will add it to exclusion list)
06:52:01.28 +00:12:01.9 -- not an asteroid (will add it to exclusion list)
06:54:05.30 -01:51:49.2 -- not an asteroid (will add it to exclusion list)
06:50:00.15 -05:55:19.3 -- not an asteroid (will add it to exclusion list)
06:44:39.20 +00:25:38.3 -- not an asteroid (will add it to exclusion list)
06:46:31.25 +01:08:36.7 -- not an asteroid (will add it to exclusion list)
06:56:04.38 -01:30:01.3 -- not an asteroid (will add it to exclusion list)
07:09:26.85 -01:56:02.1 -- not an asteroid (will add it to exclusion list)
06:47:02.80 -03:47:40.7 -- not an asteroid (will add it to exclusion list)
07:04:59.57 -03:57:33.1 -- not an asteroid (will add it to exclusion list)
07:03:36.96 -00:12:37.0 -- not an asteroid (will add it to exclusion list)
06:53:04.48 -05:33:24.5 -- not an asteroid (will add it to exclusion list)
06:58:27.05 -03:14:41.7 -- not an asteroid (will add it to exclusion list)
06:36:15.18 +01:00:10.7 -- not an asteroid (will add it to exclusion list)
06:56:16.93 +00:50:18.8 -- not an asteroid (will add it to exclusion list)
06:45:26.97 -05:18:37.3 -- not an asteroid (will add it to exclusion list)
06:52:00.95 +01:29:16.3 -- not an asteroid (will add it to exclusion list)
06:59:42.15 -02:10:53.0 -- not an asteroid (will add it to exclusion list)
06:44:14.40 +00:14:37.9 -- not an asteroid (will add it to exclusion list)
07:00:12.21 -03:47:44.1 -- not an asteroid (will add it to exclusion list)
06:58:21.12 -04:33:28.4 -- not an asteroid (will add it to exclusion list)
07:05:05.72 -03:34:37.3 -- not an asteroid (will add it to exclusion list)
06:58:39.24 +01:21:58.9 -- not an asteroid (will add it to exclusion list)
06:53:41.51 -01:02:04.6 -- not an asteroid (will add it to exclusion list)
06:54:23.77 -04:11:38.3 -- not an asteroid (will add it to exclusion list)
07:08:48.79 -03:43:03.8 -- not an asteroid (will add it to exclusion list)
07:09:41.29 -04:22:46.2 -- not an asteroid (will add it to exclusion list)
07:07:06.92 +01:40:00.1 -- not an asteroid (will add it to exclusion list)
07:03:24.80 -05:00:17.1 -- not an asteroid (will add it to exclusion list)
06:46:00.26 -00:22:07.6 -- not an asteroid (will add it to exclusion list)
07:03:25.22 -05:00:42.3 -- not an asteroid (will add it to exclusion list)
07:05:45.28 -04:50:46.5 -- not an asteroid (will add it to exclusion list)
07:08:06.96 -02:10:36.2 -- not an asteroid (will add it to exclusion list)
07:02:17.29 -03:49:25.2 -- not an asteroid (will add it to exclusion list)
06:48:31.54 -04:05:33.1 -- not an asteroid (will add it to exclusion list)
07:07:51.42 -05:47:00.1 -- not an asteroid (will add it to exclusion list)
07:09:10.53 -05:50:47.5 -- not an asteroid (will add it to exclusion list)
06:46:13.89 +00:50:42.1 -- not an asteroid (will add it to exclusion list)
07:00:12.13 -01:48:12.9 -- not an asteroid (will add it to exclusion list)
07:03:26.97 -05:01:12.8 -- not an asteroid (will add it to exclusion list)
07:09:08.45 -01:41:28.8 -- not an asteroid (will add it to exclusion list)
06:47:07.68 -01:51:11.9 -- not an asteroid (will add it to exclusion list)
06:35:07.39 -03:03:05.0 -- not an asteroid (will add it to exclusion list)
07:08:11.94 -05:47:37.9 -- not an asteroid (will add it to exclusion list)
07:05:18.17 -01:23:00.4 -- not an asteroid (will add it to exclusion list)
06:58:57.09 -03:00:41.7 -- not an asteroid (will add it to exclusion list)
06:44:34.07 -01:35:28.6 -- not an asteroid (will add it to exclusion list)
07:05:50.97 -02:05:14.3 -- not an asteroid (will add it to exclusion list)
07:09:40.01 -05:35:35.3 -- not an asteroid (will add it to exclusion list)
06:47:12.95 +00:51:23.6 -- not an asteroid (will add it to exclusion list)
06:45:12.35 -00:01:52.9 -- not an asteroid (will add it to exclusion list)
06:50:14.49 -00:47:13.2 -- not an asteroid (will add it to exclusion list)
07:06:17.14 +02:00:14.9 -- not an asteroid (will add it to exclusion list)
06:58:06.51 -01:38:10.2 -- not an asteroid (will add it to exclusion list)
06:57:11.76 -03:58:12.3 -- not an asteroid (will add it to exclusion list)
07:00:01.25 -05:09:19.7 -- not an asteroid (will add it to exclusion list)
06:54:48.40 +00:23:18.2 -- not an asteroid (will add it to exclusion list)
06:59:33.51 +01:05:00.0 -- not an asteroid (will add it to exclusion list)
06:43:47.18 +01:14:20.6 -- not an asteroid (will add it to exclusion list)
06:42:33.20 -03:28:07.2 -- not an asteroid (will add it to exclusion list)
06:42:39.02 -02:16:08.3 -- not an asteroid (will add it to exclusion list)
06:58:35.62 -04:20:28.4 -- not an asteroid (will add it to exclusion list)
06:42:42.18 -01:42:37.2 -- not an asteroid (will add it to exclusion list)
07:04:16.73 -03:01:38.5 -- not an asteroid (will add it to exclusion list)
06:41:27.06 -01:19:04.7 -- not an asteroid (will add it to exclusion list)
06:55:24.49 -05:54:32.5 -- not an asteroid (will add it to exclusion list)
06:46:50.85 +01:18:08.8 -- not an asteroid (will add it to exclusion list)
07:01:10.13 -01:01:16.0 -- not an asteroid (will add it to exclusion list)
06:40:25.87 -03:31:15.1 -- not an asteroid (will add it to exclusion list)
07:08:49.43 +00:27:13.9 -- not an asteroid (will add it to exclusion list)
06:43:42.35 -04:26:31.3 -- not an asteroid (will add it to exclusion list)
06:54:41.89 -02:41:59.1 -- not an asteroid (will add it to exclusion list)
06:49:56.14 -02:40:56.0 -- not an asteroid (will add it to exclusion list)
07:08:59.17 -00:34:33.2 -- not an asteroid (will add it to exclusion list)
06:49:07.27 -01:40:17.9 -- not an asteroid (will add it to exclusion list)
06:53:54.81 +00:47:28.6 -- not an asteroid (will add it to exclusion list)
06:44:50.72 +01:05:45.8 -- not an asteroid (will add it to exclusion list)
07:05:38.61 +01:26:02.2 -- not an asteroid (will add it to exclusion list)
06:44:48.72 +01:46:40.8 -- not an asteroid (will add it to exclusion list)
06:47:41.04 +00:31:30.9 -- not an asteroid (will add it to exclusion list)
06:47:23.73 +01:25:43.4 -- not an asteroid (will add it to exclusion list)
06:42:30.94 -06:04:22.2 -- not an asteroid (will add it to exclusion list)
07:08:37.32 +00:17:23.6 -- not an asteroid (will add it to exclusion list)
06:46:10.29 -03:14:00.3 -- not an asteroid (will add it to exclusion list)
06:41:05.36 -05:41:10.7 -- not an asteroid (will add it to exclusion list)
06:57:35.69 +01:13:53.3 -- not an asteroid (will add it to exclusion list)
07:01:28.01 -05:15:08.4 -- not an asteroid (will add it to exclusion list)
06:56:58.48 -05:23:30.6 -- not an asteroid (will add it to exclusion list)
06:49:56.02 -02:17:05.3 -- not an asteroid (will add it to exclusion list)
07:09:21.64 +01:07:25.9 -- not an asteroid (will add it to exclusion list)
06:51:34.20 -01:39:24.1 -- not an asteroid (will add it to exclusion list)
06:43:36.94 -04:25:04.0 -- not an asteroid (will add it to exclusion list)
06:52:17.74 -03:21:56.6 -- not an asteroid (will add it to exclusion list)
06:49:24.59 -00:56:18.7 -- not an asteroid (will add it to exclusion list)
07:04:51.57 -02:12:05.5 -- not an asteroid (will add it to exclusion list)
06:48:56.92 -03:30:57.8 -- not an asteroid (will add it to exclusion list)
06:50:34.17 -02:44:35.6 -- not an asteroid (will add it to exclusion list)
07:09:33.72 -04:18:54.6 -- not an asteroid (will add it to exclusion list)
06:55:18.97 +01:47:06.4 -- not an asteroid (will add it to exclusion list)
06:52:27.33 -05:52:44.1 -- not an asteroid (will add it to exclusion list)
06:55:15.88 +00:20:56.6 -- not an asteroid (will add it to exclusion list)
06:50:41.42 -00:31:46.3 -- not an asteroid (will add it to exclusion list)
07:01:35.39 -00:48:25.8 -- not an asteroid (will add it to exclusion list)
06:47:59.52 -01:20:54.5 -- not an asteroid (will add it to exclusion list)
06:59:01.98 +00:56:29.5 -- not an asteroid (will add it to exclusion list)
07:03:45.94 -02:09:36.6 -- not an asteroid (will add it to exclusion list)
06:42:15.55 +01:14:36.6 -- not an asteroid (will add it to exclusion list)
06:50:48.55 -02:55:08.6 -- not an asteroid (will add it to exclusion list)
06:48:34.57 -03:13:30.7 -- not an asteroid (will add it to exclusion list)
06:55:50.72 -02:12:29.1 -- not an asteroid (will add it to exclusion list)
06:46:52.14 +01:30:31.7 -- not an asteroid (will add it to exclusion list)
06:59:46.60 -02:22:14.2 -- not an asteroid (will add it to exclusion list)
06:53:46.48 -00:31:17.1 -- not an asteroid (will add it to exclusion list)
06:46:32.53 -01:51:13.3 -- not an asteroid (will add it to exclusion list)
06:52:50.94 -02:20:52.1 -- not an asteroid (will add it to exclusion list)
06:51:30.59 +01:15:08.1 -- not an asteroid (will add it to exclusion list)
06:52:59.48 -03:53:54.2 -- not an asteroid (will add it to exclusion list)
06:48:04.22 -01:54:53.2 -- not an asteroid (will add it to exclusion list)
06:57:11.57 -01:07:45.5 -- not an asteroid (will add it to exclusion list)
06:50:52.35 -01:26:22.7 -- not an asteroid (will add it to exclusion list)
06:52:16.18 -05:20:42.3 -- not an asteroid (will add it to exclusion list)
07:02:38.31 +01:10:27.1 -- not an asteroid (will add it to exclusion list)
06:48:22.34 -00:23:14.0 -- not an asteroid (will add it to exclusion list)
06:55:27.97 -04:33:52.7 -- not an asteroid (will add it to exclusion list)
06:41:39.95 -00:36:38.7 -- not an asteroid (will add it to exclusion list)
06:58:34.65 -01:38:22.3 -- not an asteroid (will add it to exclusion list)
06:51:28.84 -01:28:30.1 -- not an asteroid (will add it to exclusion list)
07:01:45.53 -00:36:23.0 -- not an asteroid (will add it to exclusion list)
07:08:01.12 -01:31:56.5 -- not an asteroid (will add it to exclusion list)
06:51:44.83 -03:39:24.0 -- not an asteroid (will add it to exclusion list)
06:45:19.66 +01:14:09.0 -- not an asteroid (will add it to exclusion list)
06:52:33.58 -06:13:39.8 -- not an asteroid (will add it to exclusion list)
06:44:45.95 -02:03:56.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.39 -03:03:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:15.18 +01:00:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:25.87 -03:31:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:05.36 -05:41:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.06 -01:19:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:39.95 -00:36:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:15.55 +01:14:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:30.94 -06:04:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.20 -03:28:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:39.02 -02:16:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:42.18 -01:42:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:36.94 -04:25:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:42.35 -04:26:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:47.18 +01:14:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:14.40 +00:14:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.07 -01:35:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.20 +00:25:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:45.95 -02:03:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:48.72 +01:46:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.72 +01:05:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.35 -00:01:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:13.05 -00:39:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:19.66 +01:14:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:26.97 -05:18:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:00.26 -00:22:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:10.29 -03:14:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.89 +00:50:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.25 +01:08:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:32.53 -01:51:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:50.85 +01:18:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:52.14 +01:30:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:02.80 -03:47:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:07.68 -01:51:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:12.95 +00:51:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:23.73 +01:25:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:41.04 +00:31:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.52 -01:20:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:04.22 -01:54:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:22.34 -00:23:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:31.54 -04:05:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:34.57 -03:13:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:56.92 -03:30:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.27 -01:40:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:24.59 -00:56:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.02 -02:17:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.14 -02:40:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:00.15 -05:55:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:14.49 -00:47:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:18.38 -00:09:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:34.17 -02:44:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.42 -00:31:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:48.55 -02:55:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:52.35 -01:26:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.84 -01:28:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:30.59 +01:15:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.20 -01:39:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:44.83 -03:39:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:00.95 +01:29:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:01.28 +00:12:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:16.18 -05:20:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:17.74 -03:21:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:27.33 -05:52:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:33.58 -06:13:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:50.94 -02:20:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:59.48 -03:53:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.48 -05:33:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.51 -01:02:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:46.48 -00:31:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:54.81 +00:47:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:05.30 -01:51:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:23.77 -04:11:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.89 -02:41:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.40 +00:23:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:49.12 -04:18:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:15.88 +00:20:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:18.97 +01:47:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:24.49 -05:54:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:27.97 -04:33:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.72 -02:12:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:04.38 -01:30:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:16.28 -01:49:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:16.93 +00:50:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:26.15 -02:53:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:58.48 -05:23:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.57 -01:07:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.76 -03:58:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.69 +01:13:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:06.51 -01:38:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:21.12 -04:33:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:27.05 -03:14:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.65 -01:38:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:35.62 -04:20:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.24 +01:21:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.09 -03:00:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:01.98 +00:56:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:25.27 -01:21:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:33.51 +01:05:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:42.15 -02:10:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:46.60 -02:22:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:50.22 -01:50:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:51.88 -02:58:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:01.25 -05:09:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:12.13 -01:48:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:12.21 -03:47:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:10.13 -01:01:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:28.01 -05:15:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:35.39 -00:48:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:45.53 -00:36:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.60 -04:35:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:17.29 -03:49:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:38.31 +01:10:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.80 -05:00:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.22 -05:00:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:26.97 -05:01:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.96 -00:12:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:45.94 -02:09:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.73 -03:01:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.57 -02:12:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:59.57 -03:57:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:05.72 -03:34:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:18.17 -01:23:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:38.61 +01:26:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:45.28 -04:50:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.97 -02:05:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:05.77 -01:43:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:17.14 +02:00:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.92 +01:40:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:51.42 -05:47:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:01.12 -01:31:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:06.96 -02:10:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:11.94 -05:47:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:37.32 +00:17:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.04 +01:24:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.79 -03:43:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:49.43 +00:27:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:59.17 -00:34:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:08.45 -01:41:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.53 -05:50:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.64 +01:07:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:26.85 -01:56:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:33.72 -04:18:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:40.01 -05:35:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:41.29 -04:22:46.2 -- 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)
06:35:07.39 -03:03:05.0 -- not a known variable star
06:36:15.18 +01:00:10.7 -- a known variable star
06:40:25.87 -03:31:15.1 -- not a known variable star
06:41:05.36 -05:41:10.7 -- not a known variable star
06:41:27.06 -01:19:04.7 -- a known variable star
06:41:39.95 -00:36:38.7 -- not a known variable star
06:42:15.55 +01:14:36.6 -- not a known variable star
06:42:30.94 -06:04:22.2 -- a known variable star
06:42:33.20 -03:28:07.2 -- not a known variable star
06:42:39.02 -02:16:08.3 -- not a known variable star
06:42:42.18 -01:42:37.2 -- not a known variable star
06:43:36.94 -04:25:04.0 -- a known variable star
06:43:42.35 -04:26:31.3 -- a known variable star
06:43:47.18 +01:14:20.6 -- not a known variable star
06:44:14.40 +00:14:37.9 -- not a known variable star
06:44:34.07 -01:35:28.6 -- a known variable star
06:44:39.20 +00:25:38.3 -- a known variable star
06:44:45.95 -02:03:56.6 -- not a known variable star
06:44:48.72 +01:46:40.8 -- not a known variable star
06:44:50.72 +01:05:45.8 -- not a known variable star
06:45:12.35 -00:01:52.9 -- not a known variable star
06:45:13.05 -00:39:26.7 -- not a known variable star
06:45:19.66 +01:14:09.0 -- not a known variable star
06:45:26.97 -05:18:37.3 -- not a known variable star
06:46:00.26 -00:22:07.6 -- not a known variable star
06:46:10.29 -03:14:00.3 -- a known variable star
06:46:13.89 +00:50:42.1 -- not a known variable star
06:46:31.25 +01:08:36.7 -- not a known variable star
06:46:32.53 -01:51:13.3 -- not a known variable star
06:46:50.85 +01:18:08.8 -- a known variable star
06:46:52.14 +01:30:31.7 -- not a known variable star
06:47:02.80 -03:47:40.7 -- not a known variable star
06:47:07.68 -01:51:11.9 -- not a known variable star
06:47:12.95 +00:51:23.6 -- not a known variable star
06:47:23.73 +01:25:43.4 -- a known variable star
06:47:41.04 +00:31:30.9 -- not a known variable star
06:47:59.52 -01:20:54.5 -- not a known variable star
06:48:04.22 -01:54:53.2 -- not a known variable star
06:48:22.34 -00:23:14.0 -- not a known variable star
06:48:31.54 -04:05:33.1 -- a known variable star
06:48:34.57 -03:13:30.7 -- not a known variable star
06:48:56.92 -03:30:57.8 -- not a known variable star
06:49:07.27 -01:40:17.9 -- not a known variable star
06:49:24.59 -00:56:18.7 -- not a known variable star
06:49:56.02 -02:17:05.3 -- not a known variable star
06:49:56.14 -02:40:56.0 -- not a known variable star
06:50:00.15 -05:55:19.3 -- not a known variable star
06:50:14.49 -00:47:13.2 -- not a known variable star
06:50:18.38 -00:09:33.0 -- not a known variable star
06:50:34.17 -02:44:35.6 -- not a known variable star
06:50:41.42 -00:31:46.3 -- not a known variable star
06:50:48.55 -02:55:08.6 -- a known variable star
06:50:52.35 -01:26:22.7 -- not a known variable star
06:51:28.84 -01:28:30.1 -- not a known variable star
06:51:30.59 +01:15:08.1 -- not a known variable star
06:51:34.20 -01:39:24.1 -- not a known variable star
06:51:44.83 -03:39:24.0 -- not a known variable star
06:52:00.95 +01:29:16.3 -- not a known variable star
06:52:01.28 +00:12:01.9 -- a known variable star
06:52:16.18 -05:20:42.3 -- not a known variable star
06:52:17.74 -03:21:56.6 -- not a known variable star
06:52:27.33 -05:52:44.1 -- not a known variable star
06:52:33.58 -06:13:39.8 -- not a known variable star
06:52:50.94 -02:20:52.1 -- not a known variable star
06:52:59.48 -03:53:54.2 -- not a known variable star
06:53:04.48 -05:33:24.5 -- not a known variable star
06:53:41.51 -01:02:04.6 -- a known variable star
06:53:46.48 -00:31:17.1 -- a known variable star
06:53:54.81 +00:47:28.6 -- not a known variable star
06:54:05.30 -01:51:49.2 -- not a known variable star
06:54:23.77 -04:11:38.3 -- not a known variable star
06:54:41.89 -02:41:59.1 -- not a known variable star
06:54:48.40 +00:23:18.2 -- a known variable star
06:54:49.12 -04:18:06.6 -- not a known variable star
06:55:15.88 +00:20:56.6 -- not a known variable star
06:55:18.97 +01:47:06.4 -- not a known variable star
06:55:24.49 -05:54:32.5 -- not a known variable star
06:55:27.97 -04:33:52.7 -- not a known variable star
06:55:50.72 -02:12:29.1 -- not a known variable star
06:56:04.38 -01:30:01.3 -- not a known variable star
06:56:16.28 -01:49:31.2 -- not a known variable star
06:56:16.93 +00:50:18.8 -- not a known variable star
06:56:26.15 -02:53:13.9 -- not a known variable star
06:56:58.48 -05:23:30.6 -- not a known variable star
06:57:11.57 -01:07:45.5 -- a known variable star
06:57:11.76 -03:58:12.3 -- not a known variable star
06:57:35.69 +01:13:53.3 -- a known variable star
06:58:06.51 -01:38:10.2 -- not a known variable star
06:58:21.12 -04:33:28.4 -- a known variable star
06:58:27.05 -03:14:41.7 -- not a known variable star
06:58:34.65 -01:38:22.3 -- not a known variable star
06:58:35.62 -04:20:28.4 -- not a known variable star
06:58:39.24 +01:21:58.9 -- not a known variable star
06:58:57.09 -03:00:41.7 -- not a known variable star
06:59:01.98 +00:56:29.5 -- not a known variable star
06:59:25.27 -01:21:56.3 -- not a known variable star
06:59:33.51 +01:05:00.0 -- a known variable star
06:59:42.15 -02:10:53.0 -- a known variable star
06:59:46.60 -02:22:14.2 -- not a known variable star
06:59:50.22 -01:50:12.6 -- not a known variable star
06:59:51.88 -02:58:55.2 -- not a known variable star
07:00:01.25 -05:09:19.7 -- not a known variable star
07:00:12.13 -01:48:12.9 -- not a known variable star
07:00:12.21 -03:47:44.1 -- not a known variable star
07:01:10.13 -01:01:16.0 -- not a known variable star
07:01:28.01 -05:15:08.4 -- a known variable star
07:01:35.39 -00:48:25.8 -- a known variable star
07:01:45.53 -00:36:23.0 -- not a known variable star
07:02:14.60 -04:35:51.7 -- not a known variable star
07:02:17.29 -03:49:25.2 -- not a known variable star
07:02:38.31 +01:10:27.1 -- not a known variable star
07:03:24.80 -05:00:17.1 -- a known variable star
07:03:25.22 -05:00:42.3 -- a known variable star
07:03:26.97 -05:01:12.8 -- a known variable star
07:03:36.96 -00:12:37.0 -- not a known variable star
07:03:45.94 -02:09:36.6 -- not a known variable star
07:04:16.73 -03:01:38.5 -- not a known variable star
07:04:51.57 -02:12:05.5 -- not a known variable star
07:04:59.57 -03:57:33.1 -- a known variable star
07:05:05.72 -03:34:37.3 -- not a known variable star
07:05:18.17 -01:23:00.4 -- a known variable star
07:05:38.61 +01:26:02.2 -- not a known variable star
07:05:45.28 -04:50:46.5 -- a known variable star
07:05:50.97 -02:05:14.3 -- not a known variable star
07:06:05.77 -01:43:45.8 -- not a known variable star
07:06:17.14 +02:00:14.9 -- not a known variable star
07:07:06.92 +01:40:00.1 -- not a known variable star
07:07:51.42 -05:47:00.1 -- a known variable star
07:08:01.12 -01:31:56.5 -- not a known variable star
07:08:06.96 -02:10:36.2 -- not a known variable star
07:08:11.94 -05:47:37.9 -- not a known variable star
07:08:37.32 +00:17:23.6 -- not a known variable star
07:08:43.04 +01:24:45.4 -- a known variable star
07:08:48.79 -03:43:03.8 -- not a known variable star
07:08:49.43 +00:27:13.9 -- not a known variable star
07:08:59.17 -00:34:33.2 -- a known variable star
07:09:08.45 -01:41:28.8 -- a known variable star
07:09:10.53 -05:50:47.5 -- a known variable star
07:09:21.64 +01:07:25.9 -- a known variable star
07:09:26.85 -01:56:02.1 -- a known variable star
07:09:33.72 -04:18:54.6 -- not a known variable star
07:09:40.01 -05:35:35.3 -- a known variable star
07:09:41.29 -04:22:46.2 -- not a known variable star
Found 106 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
143 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 143 (excluding asteroids and hot pixels, 106 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)2461140.65825289 -observatory V36
23:38:05.42 -04:55:32.8 Mercury (0.2mag)
02:40:21.93 +15:32:47.1 Venus (-3.9mag)
00:01:13.39 -00:57:55.6 Mars (1.2mag)
07:10:09.64 +22:50:12.0 Jupiter (-2.1mag)
00:26:33.55 +00:32:33.9 Saturn (0.9mag)
03:46:29.87 +19:43:36.8 Uranus (5.8mag)
00:10:03.95 -00:20:15.9 Neptune (7.8mag)
20:33:28.03 -22:52:27.0 Pluto (14.5mag)
19:28:41.64 -26:01:35.1 Moon (-10.4mag)
-rw-r--r-- 1 apache apache 362 Apr 9 22:51 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461140.65825289:
07:10:03.01 +22:50:23.6 Io (5.7mag)
07:10:17.88 +22:49:52.4 Europa (5.9mag)
07:10:08.62 +22:50:06.4 Ganymede (5.3mag)
07:09:47.84 +22:51:02.5 Callisto (6.6mag)
07:13:44.25 +22:40:39.3 Himalia (15.3mag)
07:10:05.58 +22:50:20.4 Thebe (16.2mag)
07:13:47.70 +23:10:10.9 Elara (17.3mag)
07:08:38.66 +23:33:15.7 Pasiphae (17.4mag)
07:18:36.81 +22:47:36.4 Carme (18.5mag)
00:26:43.39 +00:32:24.6 Titan (8.8mag)
00:26:32.51 +00:32:50.0 Rhea (10.1mag)
00:26:25.14 +00:33:37.0 Iapetus (11.5mag)
00:26:47.05 +00:32:22.5 Hyperion (14.8mag)
00:28:14.94 +00:41:59.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 22:51 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.65825289:
15:09:57.35 -11:47:32.1 JWST
19:13:17.06 +14:36:05.3 Chandra
07:55:36.19 -35:59:45.7 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 22:51 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.65825289 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:18.98 -28:26:50.3 13.9mag P/2010 H2 (Vales)
05:02:40.27 -69:56:45.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:15.88 +31:23:58.1 17.2mag C/2017 K2 (PANSTARRS)
17:30:51.36 +09:50:59.6 17.6mag C/2021 G2 (ATLAS)
23:08:34.77 +29:00:23.0 17.0mag C/2022 E2 (ATLAS)
04:22:29.35 +25:52:37.6 15.9mag C/2022 N2 (PANSTARRS)
09:02:21.11 +31:57:55.9 16.2mag C/2022 QE78 (ATLAS)
08:30:19.02 -00:47:08.5 17.3mag C/2022 R6 (PANSTARRS)
18:54:57.53 +18:02:12.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:27.32 -11:36:21.2 17.5mag P/2023 B1 (PANSTARRS)
09:10:33.70 -12:50:09.3 17.6mag C/2023 F3 (ATLAS)
21:48:02.81 +62:34:37.5 17.5mag C/2023 H5 (Lemmon)
19:23:48.71 -03:38:58.8 14.2mag C/2023 R1 (PANSTARRS)
21:40:35.12 +85:07:10.2 17.8mag C/2023 X2 (Lemmon)
06:15:34.40 +63:32:54.4 17.1mag C/2024 A1 (ATLAS)
05:00:22.03 +16:12:21.9 10.7mag C/2024 E1 (Wierzchos)
16:22:52.46 +05:25:49.8 17.4mag C/2024 G6 (ATLAS)
20:18:59.91 +13:42:43.4 14.7mag C/2024 J3 (ATLAS)
03:21:11.34 -23:17:23.3 16.4mag C/2024 T5 (ATLAS)
05:11:51.32 +46:46:37.8 17.7mag C/2025 J1 (Borisov)
14:03:04.40 +41:06:10.5 14.9mag C/2025 L1 (ATLAS)
03:16:14.48 -25:19:25.1 17.8mag C/2025 Q3 (ATLAS)
23:06:40.94 +19:42:42.5 9.4mag C/2025 R3 (PANSTARRS)
12:56:39.74 +02:38:56.4 17.5mag C/2025 Y1 (ATLAS)
02:29:48.91 +03:30:22.3 10.9mag C/2026 A1 (MAPS)
23:42:41.40 +36:05:18.3 14.4mag C/2026 B2 (Sun-Gao)
18:31:32.69 -10:01:27.8 12.2mag 10P/Tempel
15:08:02.10 +03:46:37.9 13.5mag 24P/Schaumasse
11:04:29.02 -01:43:19.5 15.7mag 29P/Schwassmann-Wachmann
17:58:48.85 -09:49:59.6 17.8mag 40P/Vaisala
10:38:06.79 -04:35:14.5 16.8mag 43P/Wolf-Harrington
01:39:38.95 +16:29:07.3 17.2mag 47P/Ashbrook-Jackson
07:00:11.76 +38:15:17.2 17.0mag 63P/Wild
23:21:31.56 -12:09:41.0 15.7mag 65P/Gunn
03:47:50.96 +19:11:52.7 15.9mag 76P/West-Kohoutek-Ikemura
00:52:43.20 +07:04:29.7 14.4mag 78P/Gehrels
22:45:03.69 -11:06:50.7 14.6mag 88P/Howell
01:54:02.44 +19:03:26.7 15.1mag 93P/Lovas
04:43:59.41 +31:57:49.8 16.3mag 123P/West-Hartley
08:21:50.50 +41:03:32.3 16.2mag 124P/Mrkos
02:24:14.28 +13:42:43.1 16.4mag 128P/Shoemaker-Holt
02:36:06.49 +13:45:58.2 17.5mag 131P/Mueller
00:55:51.87 +11:08:00.8 10.9mag 141P/Machholz
01:05:30.37 +02:40:44.3 11.0mag 141P-A/Machholz
23:53:48.44 -01:09:36.2 13.5mag 141P-D/Machholz
01:35:12.93 +04:23:58.2 17.9mag 141P-I/Machholz
00:46:07.45 -04:27:09.2 15.2mag 162P/SidingSpring
10:29:51.51 +31:15:12.1 17.9mag 164P/Christensen
06:25:42.69 +24:25:20.5 17.9mag 198P/ODAS
15:01:47.91 -00:42:41.0 17.5mag 210P/Christensen
21:21:25.98 -12:51:40.9 17.5mag 218P/LINEAR
17:14:35.87 -14:37:24.7 16.2mag 235P/LINEAR
05:21:58.69 +34:13:23.8 16.7mag 240P/NEAT
07:35:47.69 -05:49:08.7 17.7mag 242P/Spahr
15:44:45.00 +06:35:34.7 17.5mag 391P/Kowalski
07:32:06.75 +21:20:24.1 17.6mag 450P/LONEOS
05:27:27.66 +45:22:33.0 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 22:51 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 22:51 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 22:51 tns_transients_list.txt
