This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna
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,2461148.6103,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1103 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105932782956526208,2461148.6103,13.71,0.05,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
Gaia DR3 3105932782956526208 20260418.1103 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
Gaia DR3 3112307029821472512,2461148.6103,13.62,0.05,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
Gaia DR3 3112307029821472512 20260418.1103 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
ATO J102.5394-01.9046,2461148.6103,13.60,0.05,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
ATO J102.5394-01.9046 20260418.1103 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
target,2461148.6103,13.63,0.05,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
target 20260418.1103 13.63CV 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 3101124137571642112,2461148.6103,13.75,0.05,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
Gaia DR3 3101124137571642112 20260418.1103 13.75CV 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,2461148.6103,13.68,0.05,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
target 20260418.1103 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
target,2461148.6103,13.56,0.05,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
target 20260418.1103 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
target,2461148.6103,13.61,0.05,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
target 20260418.1103 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 3107886168443464320,2461148.6103,13.55,0.05,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
Gaia DR3 3107886168443464320 20260418.1103 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.88,0.05,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
target 20260418.1103 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.3710-03.8560,2461148.6103,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3710-03.8560 20260418.1103 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.63,0.05,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
target 20260418.1103 13.63CV 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 3113107165046453504,2461148.6103,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113107165046453504 20260418.1103 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.46,0.05,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
target 20260418.1103 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 J105.4041-04.5455,2461148.6103,13.59,0.05,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
ATO J105.4041-04.5455 20260418.1103 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
target,2461148.6103,13.41,0.05,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
target 20260418.1103 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
Gaia DR3 3112299500737047808,2461148.6103,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112299500737047808 20260418.1103 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107119602680173696,2461148.6103,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3107119602680173696 20260418.1103 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111243252318949248,2461148.6103,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111243252318949248 20260418.1103 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126184240951801216,2461148.6103,13.40,0.05,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 3126184240951801216 20260418.1103 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,2461148.6103,13.37,0.05,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 20260418.1103 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,2461148.6103,13.54,0.05,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 20260418.1103 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107647265186582528,2461148.6103,13.30,0.05,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
Gaia DR3 3107647265186582528 20260418.1103 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
ASASSN-V J064630.95+010809.2,2461148.6103,13.40,0.05,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
ASASSN-V J064630.95+010809.2 20260418.1103 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,2461148.6103,13.31,0.05,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 20260418.1103 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.4938-02.8215,2461148.6103,13.36,0.05,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
ATO J106.4938-02.8215 20260418.1103 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100611352837987968,2461148.6103,13.27,0.05,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 3100611352837987968 20260418.1103 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
Gaia DR3 3107879640093284736,2461148.6103,13.38,0.05,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
Gaia DR3 3107879640093284736 20260418.1103 13.38CV 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,2461148.6103,13.38,0.05,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
target 20260418.1103 13.38CV 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
ATO J104.0605-03.8344,2461148.6103,13.34,0.05,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 J104.0605-03.8344 20260418.1103 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,2461148.6103,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1103 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107171584665401984,2461148.6103,13.41,0.05,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
Gaia DR3 3107171584665401984 20260418.1103 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,2461148.6103,13.06,0.05,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
target 20260418.1103 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 3108860782423215232,2461148.6103,13.34,0.05,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 3108860782423215232 20260418.1103 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,2461148.6103,13.31,0.05,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 20260418.1103 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,2461148.6103,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1103 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109005952316009984,2461148.6103,13.12,0.05,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 3109005952316009984 20260418.1103 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,2461148.6103,13.07,0.05,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 20260418.1103 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 3101676264206730240,2461148.6103,13.22,0.05,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 3101676264206730240 20260418.1103 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 J105.3524-01.2303,2461148.6103,13.12,0.05,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 J105.3524-01.2303 20260418.1103 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 3112469585742136064,2461148.6103,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112469585742136064 20260418.1103 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.03,0.05,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 20260418.1103 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 3126221658707146368,2461148.6103,12.78,0.05,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 3126221658707146368 20260418.1103 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 3114460526421262848,2461148.6103,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260418.1103 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3101279508008034560,2461148.6103,12.88,0.05,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 3101279508008034560 20260418.1103 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9152-04.6412,2461148.6103,12.89,0.05,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
ATO J105.9152-04.6412 20260418.1103 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,12.94,0.05,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 20260418.1103 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
Mean magnitude and position on the discovery images:
2026 04 18.1103 2461148.6103 12.81 06:50:27.80 -05:47:26.4
217.97901 -2.85287 galactic Mon Second-epoch detections are separated by 0.2" and 2.5 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 3101861184018583168 | 06:50:27.80 -05:47:26.4 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: A6V 2012A&A...541A..34S CoRoT 110747337
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 3101861184018583168,2461148.6103,12.81,0.05,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
Large-amplitude variable Gaia DR2 3101861184018583168 20260418.1103 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
target,2461148.6103,12.82,0.05,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 20260418.1103 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.8410-02.4767,2461148.6103,12.56,0.05,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
ATO J105.8410-02.4767 20260418.1103 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 3100850496619907072,2461148.6103,12.73,0.05,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
Gaia DR3 3100850496619907072 20260418.1103 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.1777-02.2246,2461148.6103,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.1777-02.2246 20260418.1103 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105924742777831040,2461148.6103,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105924742777831040 20260418.1103 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053304074782543488,2461148.6103,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053304074782543488 20260418.1103 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102372667384237952,2461148.6103,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102372667384237952 20260418.1103 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,12.62,0.05,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
target 20260418.1103 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125569957548660864,2461148.6103,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125569957548660864 20260418.1103 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7797-03.0546,2461148.6103,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260418.1103 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
target,2461148.6103,12.40,0.05,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
target 20260418.1103 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,2461148.6103,12.13,0.05,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
target 20260418.1103 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
Gaia DR3 3053389149496017280,2461148.6103,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053389149496017280 20260418.1103 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112051973180962048,2461148.6103,11.46,0.05,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
Gaia DR3 3112051973180962048 20260418.1103 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065134.58+002720.2,2461148.6103,11.36,0.05,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
ZTF J065134.58+002720.2 20260418.1103 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3071-00.0429,2461148.6103,10.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3071-00.0429 20260418.1103 10.52CV 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 J106.5593+02.0025,2461148.6103,11.71,0.05,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 J106.5593+02.0025 20260418.1103 11.71CV 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
Gaia DR3 3105345059631344768,2461148.6103,12.07,0.05,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
Gaia DR3 3105345059631344768 20260418.1103 12.07CV 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 3112551941736184448,2461148.6103,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112551941736184448 20260418.1103 12.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9580+01.5948,2461148.6103,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9580+01.5948 20260418.1103 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 J106.6984-06.0641,2461148.6103,12.62,0.05,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 J106.6984-06.0641 20260418.1103 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112424230887731712,2461148.6103,12.54,0.05,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 3112424230887731712 20260418.1103 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 3053416980884797824,2461148.6103,12.55,0.05,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
Gaia DR3 3053416980884797824 20260418.1103 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125504223071142784,2461148.6103,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125504223071142784 20260418.1103 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065448.56+002321.1,2461148.6103,12.62,0.05,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
ZTF J065448.56+002321.1 20260418.1103 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 J100.6477-03.4721,2461148.6103,12.69,0.05,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
ATO J100.6477-03.4721 20260418.1103 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,2461148.6103,12.73,0.05,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 20260418.1103 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461148.6103,12.78,0.05,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
ATO J106.0676-03.0161 20260418.1103 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.5494+00.3110,2461148.6103,12.75,0.05,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 J106.5494+00.3110 20260418.1103 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
ATO J104.2998-03.9607,2461148.6103,12.76,0.05,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
ATO J104.2998-03.9607 20260418.1103 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 3106340014576032512,2461148.6103,12.77,0.05,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
Gaia DR3 3106340014576032512 20260418.1103 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 3105921684761121152,2461148.6103,12.77,0.05,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
Gaia DR3 3105921684761121152 20260418.1103 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
target,2461148.6103,12.83,0.05,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 20260418.1103 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 3053393715036723840,2461148.6103,12.85,0.05,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
Gaia DR3 3053393715036723840 20260418.1103 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105947282767695360,2461148.6103,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105947282767695360 20260418.1103 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,12.84,0.05,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
target 20260418.1103 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
target,2461148.6103,12.93,0.05,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
target 20260418.1103 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 3126153111029053568,2461148.6103,12.89,0.05,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 3126153111029053568 20260418.1103 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_J0651481-040224,2461148.6103,12.96,0.05,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
GDS_J0651481-040224 20260418.1103 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,2461148.6103,13.01,0.05,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
target 20260418.1103 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 J106.1044-05.1304,2461148.6103,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1044-05.1304 20260418.1103 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9043-01.6544,2461148.6103,12.97,0.05,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
ATO J102.9043-01.6544 20260418.1103 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
Gaia DR3 3106035656015561472,2461148.6103,13.02,0.05,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 3106035656015561472 20260418.1103 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
CoRoT 102806577,2461148.6103,13.04,0.05,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
CoRoT 102806577 20260418.1103 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,2461148.6103,12.95,0.05,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
target 20260418.1103 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
Gaia DR3 3113219246514568576,2461148.6103,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260418.1103 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0649315-012934,2461148.6103,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0649315-012934 20260418.1103 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.05,0.05,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
target 20260418.1103 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 3108798488219749888,2461148.6103,13.08,0.05,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 3108798488219749888 20260418.1103 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
GDS_J0703252-030259,2461148.6103,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0703252-030259 20260418.1103 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105302831513609216,2461148.6103,13.06,0.05,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
Gaia DR3 3105302831513609216 20260418.1103 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 3100429448080531584,2461148.6103,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100429448080531584 20260418.1103 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109656416522583808,2461148.6103,12.91,0.05,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 20260418.1103 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108917372911018368,2461148.6103,13.01,0.05,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 3108917372911018368 20260418.1103 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 J099.6630+01.9547,2461148.6103,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.6630+01.9547 20260418.1103 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113470691079092224,2461148.6103,13.11,0.05,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
Gaia DR3 3113470691079092224 20260418.1103 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
Gaia DR3 3112852799904385536,2461148.6103,13.18,0.05,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
Gaia DR3 3112852799904385536 20260418.1103 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100477590376004224,2461148.6103,13.03,0.05,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 3100477590376004224 20260418.1103 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 3113580985840495488,2461148.6103,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113580985840495488 20260418.1103 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.5152-01.3222,2461148.6103,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.5152-01.3222 20260418.1103 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107281540128223104,2461148.6103,13.05,0.05,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 3107281540128223104 20260418.1103 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 3106113274662574208,2461148.6103,13.22,0.05,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 3106113274662574208 20260418.1103 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,2461148.6103,13.16,0.05,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
target 20260418.1103 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
Gaia DR3 3113700076693885568,2461148.6103,13.15,0.05,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 3113700076693885568 20260418.1103 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 3113390186212355840,2461148.6103,13.12,0.05,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 3113390186212355840 20260418.1103 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,2461148.6103,13.14,0.05,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
target 20260418.1103 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.20,0.05,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 20260418.1103 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6624+00.2039,2461148.6103,13.05,0.05,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
ATO J103.6624+00.2039 20260418.1103 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461148.6103,13.12,0.05,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 J101.9913-01.3476 20260418.1103 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 3113913996125565440,2461148.6103,13.03,0.05,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 3113913996125565440 20260418.1103 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 3100349974007792000,2461148.6103,13.33,0.05,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 3100349974007792000 20260418.1103 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106229822896913792,2461148.6103,13.27,0.05,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 3106229822896913792 20260418.1103 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
Gaia DR3 3112223325200684160,2461148.6103,13.27,0.05,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 3112223325200684160 20260418.1103 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
Gaia DR3 3106318947754976512,2461148.6103,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106318947754976512 20260418.1103 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2307+00.9114,2461148.6103,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.2307+00.9114 20260418.1103 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109579137170282880,2461148.6103,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109579137170282880 20260418.1103 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100441267835993600,2461148.6103,13.30,0.05,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
Gaia DR3 3100441267835993600 20260418.1103 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
ASAS J065055-0458.5,2461148.6103,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J065055-0458.5 20260418.1103 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107246630634720768,2461148.6103,13.31,0.05,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
Gaia DR3 3107246630634720768 20260418.1103 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 3105909968090861824,2461148.6103,13.36,0.05,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 3105909968090861824 20260418.1103 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101146368322338688,2461148.6103,13.37,0.05,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
Gaia DR3 3101146368322338688 20260418.1103 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
ATO J103.4997-02.1281,2461148.6103,13.37,0.05,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 J103.4997-02.1281 20260418.1103 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
ATO J104.8095-01.6362,2461148.6103,13.27,0.05,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
ATO J104.8095-01.6362 20260418.1103 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
Gaia DR3 3102841437296883840,2461148.6103,13.36,0.05,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 3102841437296883840 20260418.1103 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126343429620148736,2461148.6103,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3126343429620148736 20260418.1103 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.30,0.05,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
target 20260418.1103 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
Gaia DR3 3107452067507929344,2461148.6103,13.54,0.05,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
Gaia DR3 3107452067507929344 20260418.1103 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106021564222428032,2461148.6103,13.38,0.05,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
Gaia DR3 3106021564222428032 20260418.1103 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109192074721221376,2461148.6103,13.36,0.05,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 3109192074721221376 20260418.1103 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.27,0.05,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
target 20260418.1103 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
target,2461148.6103,13.38,0.05,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
target 20260418.1103 13.38CV 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
ATO J103.1185-02.6809,2461148.6103,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.1185-02.6809 20260418.1103 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105590967980076416,2461148.6103,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3105590967980076416 20260418.1103 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4491-02.6658,2461148.6103,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4491-02.6658 20260418.1103 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
ATO J102.3653-03.1347,2461148.6103,13.81,0.05,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 J102.3653-03.1347 20260418.1103 13.81CV 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 J102.1645+01.9540,2461148.6103,13.59,0.05,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
ATO J102.1645+01.9540 20260418.1103 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 J103.0736-03.3663,2461148.6103,13.54,0.05,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
ATO J103.0736-03.3663 20260418.1103 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108459460677899520,2461148.6103,13.44,0.05,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
Gaia DR3 3108459460677899520 20260418.1103 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
ATO J104.6381-01.6369,2461148.6103,13.52,0.05,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 J104.6381-01.6369 20260418.1103 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.61,0.05,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
target 20260418.1103 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
target,2461148.6103,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1103 13.77CV 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
target,2461148.6103,13.62,0.05,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
target 20260418.1103 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
Gaia DR3 3113071460980262528,2461148.6103,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3113071460980262528 20260418.1103 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6103,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1103 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101786623387963264,2461148.6103,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3101786623387963264 20260418.1103 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0648234-002937,2461148.6103,13.68,0.05,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
GDS_J0648234-002937 20260418.1103 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
Gaia DR3 3125539824058820480,2461148.6103,13.67,0.05,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
Gaia DR3 3125539824058820480 20260418.1103 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
ATO J105.3509-05.4361,2461148.6103,13.94,0.05,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 J105.3509-05.4361 20260418.1103 13.94CV 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
## 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: 2461148.61059376 18.04.2026 02:39:05.301 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
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: 13 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): 31503
Objects passed selection criteria: 31397
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 25311.8
Average stars matched: 22918.2 (90.5439 %)
Memory usage VmPeak: 131772 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 21:54:20 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: 2461148.61059376 18.04.2026 02:39:05.301 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 395
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: 304 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): 227792
Objects passed selection criteria: 227045
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 186036
Average stars matched: 169228 (90.9653 %)
Memory usage VmPeak: 2021224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 22:01:20 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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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: 2461148.61008652
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:20.623 -02:01:19.66 J2000 4789.000 3195.000
###################################
###################################
# 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 06:51:20.623 -02:01:19.66
Angular distance between the image centers 0.0951 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:19.875 -02:01:28.47 J2000 4789.000 3195.000
###################################
###################################
# 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 06:51:19.875 -02:01:28.47
Angular distance between the image centers 0.0987 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 06:51:20.623 -02:01:19.66
Second-epoch second image center 06:51:19.875 -02:01:28.47
Angular distance between the image centers 0.00396 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.f6la2GEIJW
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.4aXPOKic5u
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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits &> /tmp/tmp.MTjFzPDGZO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits &> /tmp/tmp.C9FKnIioFb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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 12 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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.f6la2GEIJW (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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.4aXPOKic5u (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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.MTjFzPDGZO (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3006, passed=28914
Got 28914 stars (including 25880 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 28914 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 28446 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 28444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 28444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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.C9FKnIioFb (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2879, passed=29074
Got 29074 stars (including 26179 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 29074 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 28596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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 -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 28597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 28596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57805.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 51876_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 51876_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:53.37 +00:28:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.059 3113576106757812864 102.97217665174 +00.47483825756 12.3842 12.1239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51882_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 51882_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:07.44 -01:28:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 2.810 3106909213700454528 099.53163508451 -01.46839862892 11.0128 10.8637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 54363_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 54363_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:13.62 -02:21:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55013_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 55013_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:37.25 -03:49:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56722_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 56722_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:44:47.52 -05:17:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57004_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 57004_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:01:12.77 -02:20:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.093 3108942146282633344 105.30290455146 -02.33807935328 12.1057 11.3156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57028_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 57028_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:09.62 -02:35:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.314 3105917355433930880 102.79000853321 -02.59546837364 11.5920 10.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57190_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 57190_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:36:17.86 -05:48:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.934 3103232515541099520 099.07422740853 -05.81032084959 11.4256 10.3522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57256_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 57256_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:37.43 -02:54:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.159 3105716488402867584 101.65586277502 -02.90978906622 11.4636 10.2931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57779_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 57779_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:40.18 -03:16:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.005 3105807541711416448 102.91751408594 -03.27792843480 12.0078 11.8525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57805_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 57805_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:43:57.66 -05:05:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.210 3100715669003273088 100.99050597606 -05.08366354313 11.8817 11.3420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58021_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 58021_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:37.69 +00:43:02.7 in the exclusion list exclusion_list.txt ****
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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:20.623 -02:01:19.66 J2000 4789.000 3195.000
###################################
###################################
# 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 06:51:20.623 -02:01:19.66
Angular distance between the image centers 0.0951 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:19.875 -02:01:28.47 J2000 4789.000 3195.000
###################################
###################################
# 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 06:51:19.875 -02:01:28.47
Angular distance between the image centers 0.0987 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 06:51:20.623 -02:01:19.66
Second-epoch second image center 06:51:19.875 -02:01:28.47
Angular distance between the image centers 0.00396 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.YjqOKIO94r
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.zQud9kXGaO
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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits &> /tmp/tmp.7Tqd1peSHi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits &> /tmp/tmp.LORMFTKTQ2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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 341 candidate transients before the final filtering. (Hard limit: 8000)
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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
2.4 pix fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (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.YjqOKIO94r (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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.zQud9kXGaO (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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.7Tqd1peSHi (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=71, blended=30292, passed=196984
Got 196984 stars (including 166484 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 196984 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 194314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 194315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 194316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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.LORMFTKTQ2 (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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=29451, passed=191541
Got 191541 stars (including 161895 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 191541 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 188201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 188201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 188200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/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_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-38-21_20.00sec_-5.00C_LIGHT_0030.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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_2026-04-17_CI_Mon-02-Q2b1x1_214935_TTUQ2b1x1_493333_M1fSiCna/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031.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
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out283611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283752.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__out283810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283823.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out283958.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out283965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284038.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out307267.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out311118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311893.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out312580.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out314700.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out315209.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out315330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out317955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318604.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out318658.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out319060.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out320593.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out325055.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_apass.txt__out323760.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out326100.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out283608.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out319734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320486.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324584.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325676.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326605.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 189s
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: 106s
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Considering the candidate 283608_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283608_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283611_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283611_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:41:19.83 +00:34:07.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 283612_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283612_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283615_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283615_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283624_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283624_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283636_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283636_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283637_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283637_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:05:01.42 -03:47:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.476 3107793809467159040 106.25531322015 -03.79847718767 14.3805 13.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283640_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283640_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:06:02.89 -02:23:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.349 3108806081720568448 106.51173366324 -02.39311255403 14.3822 13.5840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283647_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283647_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:16.66 -06:10:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.144 3053091010044497280 107.31940521770 -06.17992875142 14.2259 13.4204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283656_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283656_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:05:50.14 -01:38:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.359 3109274679831101184 106.45821982357 -01.63871250965 14.2250 13.4102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283661_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283661_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283664_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283664_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283667_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283667_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283673_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283673_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283678_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283678_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:35.72 -00:47:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.630 3113153104019358208 102.89838238603 -00.79632488196 14.3648 13.4353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283690_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283690_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283699_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283699_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:48.99 -01:46:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.101 3109088175171141632 105.70361971433 -01.77817000677 14.4731 14.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283700_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:36:03.55 -01:51:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.895 3118787688791853952 099.01461995362 -01.85606814139 14.2984 13.3105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283718_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283718_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:16.85 -00:08:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 4.220 3111219161843472000 107.07096844253 -00.13928126402 14.3963 13.9222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283719_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283719_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283721_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283721_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:01:08.47 -05:31:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.606 3101364587024900480 105.28475188659 -05.52756864355 14.5694 14.0918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283724_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283724_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:05.78 +01:36:29.3 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 283725_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283725_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283731_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283731_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283738_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283738_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:59:25.36 -02:10:14.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 283739_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283739_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:09.31 +00:44:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.836 3125644724339983744 101.78871008674 +00.74104857530 14.2112 13.6608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283741_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283741_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283742_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283742_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283747_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283747_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283751_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283751_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:45:11.73 +00:14:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.788 3125505739198071040 101.29884931989 +00.24208721242 14.2269 13.7415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283752_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283752_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:36:42.94 -00:41:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.316 3119022640682440832 099.17974755221 -00.68978084683 14.2986 13.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283768_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283768_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283779_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283779_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283780_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283780_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 283781_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283781_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283783_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283783_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283787_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283787_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283794_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283794_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283800_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283800_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283803_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:20.73 -00:17:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.911 3107460343905382912 101.58623755812 -00.28548509265 14.2042 13.5171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283806_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283806_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:05:16.05 -05:50:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.156 3053267412943732480 106.31632121050 -05.84842925565 14.3145 13.9047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283810_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283810_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:01:19.91 -00:56:39.1 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 283811_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283811_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:05:58.84 +00:11:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.843 3112759547573659008 106.49478838253 +00.18855727320 14.1112 13.5262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283817_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283817_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283823_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283823_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:12.63 -04:22:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.148 3101742406704701312 105.55273884360 -04.36882587785 14.2554 13.7313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283828_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283828_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:50:48.82 +00:23:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.276 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283837_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283837_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283839_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283839_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 283842_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283842_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283868_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283868_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:59:51.10 -05:12:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.208 3101581706207521280 104.96246888320 -05.20313260263 13.9922 13.4966 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#
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Considering the candidate 283872_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283872_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283876_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283876_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:19.05 -01:02:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.101 3109413218295766400 107.32904768222 -01.03529667759 14.0534 13.5389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283877_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283877_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:01:25.19 -00:51:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 4.046 3112572012122478976 105.35435761923 -00.86556119454 14.1848 13.5538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283882_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283882_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283896_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283896_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:43:01.07 +00:24:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.803 3119569196745019136 100.75433837111 +00.40826370389 14.1656 13.7134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283899_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283899_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283904_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283904_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 283912_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283912_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283917_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283917_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:50:48.37 -01:23:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.826 3106350013260096256 102.70086659772 -01.39981760964 14.0145 13.7108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283920_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283920_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283922_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283922_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:48:52.60 +00:01:16.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283933_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283933_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:05:25.30 -03:36:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.438 3107820060307074816 106.35605107274 -03.60946233271 13.9552 13.1959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283934_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283934_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283935_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283935_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:50:24.02 -01:20:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.176 3106354303926910336 102.59964143886 -01.34599586524 14.0492 13.4869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283945_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:33.65 -01:57:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.008 3109049314307207680 105.63950162813 -01.96758727063 13.9169 13.1322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.008#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283949_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283949_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:12.36 -02:00:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.902 3106057504510134144 103.55142824856 -02.00219018737 13.8583 12.9554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.902#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283950_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:45.10 -03:41:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.561 3107703821317850368 107.43704622586 -03.69891737982 13.8124 13.3638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283958_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:03:24.15 +01:44:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.161 3115407858769508864 105.85054732941 +01.73724252246 13.7366 12.8891 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 283961_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283961_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:50.01 +00:33:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.433 3113616548169343104 102.45804111476 +00.55027335106 13.6126 12.7223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283965_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283965_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:03.92 -01:19:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.478 3109387482852637312 107.26623640237 -01.32634810055 13.6962 13.0876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283966_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283966_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283970_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 283970_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:43:04.69 +01:03:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.659 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283976_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283976_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283983_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283983_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283995_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283995_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 283997_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 283997_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284000_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:00:52.15 +01:33:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.414 3115389132712944384 105.21749876504 +01.55266609547 13.3442 12.3040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284013_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284013_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:37.55 -02:21:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.385 3106690204730551936 099.65602265592 -02.35585984284 13.2484 12.1574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284015_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284015_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284016_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284016_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284023_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284023_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284028_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284028_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284038_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284038_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:44:18.23 -05:27:36.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 284046_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284046_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284047_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284047_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:48:49.85 +00:22:48.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
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Considering the candidate 284049_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284049_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284052_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284052_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284055_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284055_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:43.49 +01:59:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.366 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284058_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284058_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284062_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284062_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:07:25.39 +02:12:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.314 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284069_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284069_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284075_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284075_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284078_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284078_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:12.64 +00:51:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284083_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284083_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:57:53.29 -00:24:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.358 3112475323818314752 104.47188036842 -00.41113470113 13.3040 12.4449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284087_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284087_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:53.99 +01:48:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.076 3114192550524702208 103.47481321244 +01.81526900993 13.1717 12.7564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284088_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284088_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284094_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284094_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:09.76 -03:38:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 2.637 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284097_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284097_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:23.16 +01:06:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.843 3125681317461063680 102.34631436143 +01.10589895291 13.1953 12.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284102_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284102_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:08.76 +00:42:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 2.488 3113634243433657472 102.28627901066 +00.71284521586 13.1110 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284110_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284110_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284112_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:13.57 +01:34:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.398 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284114_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284114_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284116_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284116_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:02.43 +01:07:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284118_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284118_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:08.26 -05:53:00.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 284124_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284124_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:04:15.78 -02:22:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284129_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284129_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:50.75 +01:53:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284131_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284131_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:11.76 -01:33:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284132_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284132_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284134_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284134_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:35.64 +01:46:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 284137_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 284137_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 284142_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 284142_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:07:49.50 -05:43:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 285323_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 285323_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 287081_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 287081_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 288697_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 288697_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:37.25 +00:26:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288944_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 288944_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:48:15.60 +01:46:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289253_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 289253_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:39.74 +00:25:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289974_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 289974_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:37.71 +00:43:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290748_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 290748_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:30.55 -01:04:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291684_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 291684_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 291749_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 291749_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:50:41.63 -00:33:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291822_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 291822_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:11.30 -06:02:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292460_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 292460_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 293306_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 293306_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 294293_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 294293_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:03:11.93 -02:15:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 295590_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 295590_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 297386_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 297386_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:50:44.42 -00:31:37.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 298053_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 298053_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:39.56 -04:37:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298062_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 298062_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 298612_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 298612_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:45:00.21 -00:03:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299308_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 299308_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:03.38 -02:29:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.366 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300151_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 300151_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:23.04 +00:25:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.890 3113001715010265856 105.59586879156 +00.43145813945 12.8711 12.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300491_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 300491_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:34:15.06 -05:19:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.126 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300498_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 300498_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:06:42.32 -03:09:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.437 3107979111536590592 106.67588059035 -03.15417042601 13.0043 12.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300548_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 300548_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 300598_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 300598_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:54.28 +00:00:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.995 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 300815_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 300815_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:15.18 -05:59:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300972_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 300972_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:07:31.13 +00:46:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 2.591 3114351331172456192 106.87951415988 +00.76727923449 12.7081 11.6609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 301243_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 301243_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:17.55 -04:25:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.406 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303044_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 303044_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:06:30.48 -06:00:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303340_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 303340_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 303546_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 303546_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 303625_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 303625_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:17.66 -03:14:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.305 3108624696661653888 105.57310754703 -03.24292917899 13.4515 12.7613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 303842_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 303842_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:03.35 -06:07:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304157_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 304157_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:07.35 -01:52:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304174_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 304174_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:03.82 -03:46:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 304280_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 304280_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 304311_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 304311_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 304759_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 304759_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:19.83 -03:22:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.994 3105616604643085952 100.08227451735 -03.38133788963 13.4827 13.0462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 304798_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 304798_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 305256_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 305256_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:52:55.11 -02:23:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.142 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305499_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 305499_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 305624_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 305624_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 305726_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 305726_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:36.01 +01:59:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306198_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 306198_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:39.15 -02:16:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306715_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 306715_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:23.34 -01:37:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.297 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306840_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 306840_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:14.74 -02:18:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.156 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306846_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 306846_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:45:06.14 -00:02:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 2.450 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307220_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 307220_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:00:53.38 +02:12:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.049 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307267_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 307267_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:52:14.05 -00:06:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.918 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307429_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 307429_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:41:18.57 -00:51:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.096 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307642_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 307642_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 308145_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 308145_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 308157_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 308157_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 308282_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 308282_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 308516_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 308516_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:01:10.31 -01:01:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.739 3112567987734134144 105.29366963077 -01.02124268361 13.7541 13.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308790_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 308790_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 308832_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 308832_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 308982_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 308982_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 309224_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 309224_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:59.66 -02:44:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.463 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309360_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 309360_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 309720_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 309720_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 309949_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 309949_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:48:33.41 +01:51:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310037_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 310037_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 310109_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 310109_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:48:20.56 -00:31:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310155_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 310155_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 310239_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 310239_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 310240_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 310240_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:56:43.18 +02:11:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310405_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 310405_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 310708_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 310708_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 310921_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 310921_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 310991_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 310991_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 311118_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 311118_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:51:26.30 -02:20:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.854 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311156_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 311156_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 311195_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 311195_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:50.65 +01:18:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 3.707 3125737976669232256 101.71061901697 +01.30128313633 13.9023 13.1882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311893_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 311893_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:48:21.02 -03:11:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.662 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312303_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 312303_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 312371_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 312371_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 312409_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 312409_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:59.52 -01:03:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.022 3112333791758054272 103.74773607348 -01.05207476769 13.3921 12.4083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312580_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 312580_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:05.27 -04:41:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.622 3103780042268573568 100.02241043894 -04.69454432899 13.8502 13.0386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312584_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 312584_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 312610_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 312610_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 312700_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 312700_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 312846_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 312846_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:46.53 -02:44:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.841 3106508927049985280 100.69338451398 -02.73839649824 13.7626 13.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313137_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 313137_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 313185_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 313185_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 313223_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313223_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:04:05.01 -02:22:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.291 3108833221613004800 106.02064200889 -02.37978674497 13.9010 13.5534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313276_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 313276_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 313317_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313317_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:55:24.48 -05:54:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 313357_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313357_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:49.45 +00:27:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.329 3114279519319862400 107.20543385668 +00.45405634620 13.8903 13.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313380_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313380_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:09.60 -05:17:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.558 3100639871420927872 101.78975441255 -05.28971896782 13.7735 12.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313420_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313420_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:41:05.48 -05:41:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.213 3100575683127182848 100.27197276181 -05.68650192790 13.9287 13.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313497_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313497_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:01:28.07 -05:15:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.072 3101401729901841408 105.36605808833 -05.25268963173 13.9656 13.5006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313625_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 313625_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 313628_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 313628_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:58:26.09 -05:48:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.483 3100992264898211584 104.60868983330 -05.80991184590 14.0487 13.5345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313660_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 313660_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 314105_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 314105_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 314305_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 314305_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 314418_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 314418_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:06:54.15 +02:10:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 314522_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 314522_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:55:58.71 -01:35:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.768 3112099187762874112 103.99454201873 -01.60068098726 13.8572 13.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314558_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 314558_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 314680_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 314680_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 314700_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 314700_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:13.91 -04:35:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.059 3102106757370145024 103.30765488832 -04.59815503995 14.0964 13.6831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314715_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 314715_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:40.16 -00:26:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.705 3112511367183611136 103.66730236160 -00.44919517720 13.9757 13.1957 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 314729_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 314729_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:29.71 -04:08:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.016 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314863_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 314863_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 314962_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 314962_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 315209_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315209_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:58.51 -00:30:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 5.201 3119415711793096832 099.74273250352 -00.50489919050 13.6777 12.6099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315258_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315258_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:42:15.46 +01:14:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.824 3125885414305835648 100.56374559839 +01.24197894342 13.9411 13.1211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315330_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315330_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:22.93 -02:46:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.139 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315342_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315342_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:28.84 -06:01:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.392 3103166480420332032 099.61974936398 -06.02795289401 13.7856 12.9545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315654_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315654_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:04.12 +01:58:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315725_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 315725_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 315767_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 315767_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 315778_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315778_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:20.44 -05:15:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.330 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315799_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315799_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:39:08.74 -03:48:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.378 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315809_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315809_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:03:07.00 +01:49:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315966_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 315966_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 315983_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 315983_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:52.44 +01:12:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.768 3120620024919006848 099.71870063274 +01.20611895865 14.1237 13.6672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316091_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 316091_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 316177_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 316177_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:52:27.36 -05:52:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.728 3101108916207784960 103.11340523708 -05.87976646569 14.0840 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316572_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 316572_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 316933_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 316933_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:04.56 -01:43:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.410 3109233104548149120 107.01874958326 -01.72878742697 13.9560 13.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317078_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 317078_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 317079_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 317079_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:45.47 +01:25:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.074 3114076418906304512 103.43838803221 +01.42863147043 14.0414 13.1455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317103_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 317103_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 317136_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 317136_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 317146_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 317146_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 317178_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 317178_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 317194_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 317194_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 317280_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 317280_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 317642_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 317642_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:57.52 -02:12:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.667 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317815_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 317815_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:27.57 -05:04:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.137 3102156029234873472 101.86457739760 -05.08341579408 14.1265 13.5611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317955_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 317955_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:03:46.82 -01:04:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.031 3109553199868724224 105.94499944489 -01.08113492279 14.0995 13.5489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318011_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 318011_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:54:17.86 -04:54:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.672 3102036148108303488 103.57398469743 -04.91417479959 14.1319 13.6028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318154_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318154_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318383_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318383_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318409_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318409_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318446_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318446_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318585_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318585_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318604_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 318604_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:14.68 -03:39:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.969 3105452708691209216 101.81087051013 -03.65148798860 13.4646 12.2211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318612_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 318612_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:06:14.87 -04:55:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.136 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318658_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 318658_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:24.59 -00:56:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.740 3107130769594752128 102.35183201837 -00.93873825599 14.2056 13.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318746_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 318746_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:03:39.65 -00:16:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.670 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318766_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318766_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318780_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318780_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318829_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318829_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 318999_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 318999_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 319060_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 319060_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:45:33.71 -00:26:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.198 3107451723910491520 101.39020146722 -00.43924863840 14.0394 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319417_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 319417_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:22.42 +01:18:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.559 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319448_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 319448_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 319538_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 319538_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 319676_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 319676_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 319707_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 319707_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 319734_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 319734_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 320486_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 320486_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 320593_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 320593_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:49:38.82 +00:36:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.291 3113619949783427072 102.41144535065 +00.61020120759 13.8962 12.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320762_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 320762_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 320990_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 320990_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 321056_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 321056_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 321099_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 321099_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:45:24.53 -02:02:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.470 3106935846799955712 101.35189817049 -02.04941269651 14.3338 13.8621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321428_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 321428_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:34:54.45 +01:23:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.968 3120676855925773696 098.72578573357 +01.39802428046 13.2177 11.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.968#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321453_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 321453_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 321467_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 321467_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 321734_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 321734_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:13.78 -05:27:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 5.070 3100630594291784192 101.55802271223 -05.45858847386 14.0725 13.1686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321824_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 321824_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 321834_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 321834_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 321953_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 321953_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:33:29.00 +01:58:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.195 3120965610869943424 098.36990336847 +01.97793607089 13.8185 12.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322144_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 322144_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:47:28.81 -01:01:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.180 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322149_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 322149_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 322370_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 322370_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:53.37 -00:49:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.779 3119330641377186688 099.72224575617 -00.82187219144 14.2480 13.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322477_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 322477_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 322655_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 322655_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:46:39.57 -05:23:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.728 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322744_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 322744_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 322862_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 322862_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 322868_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 322868_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 323057_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 323057_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 323127_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 323127_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:53:42.42 -04:35:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.698 3102104695785792640 103.42597967893 -04.59345645621 14.4577 13.4011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323760_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 323760_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:40.07 -02:15:36.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 323790_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 323790_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:38:10.03 +01:23:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.977 3120638098141033728 099.54150956921 +01.38300044165 14.4812 13.7446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324013_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 324013_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 324076_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 324076_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:55:11.29 -05:51:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.558 3101074002414434304 103.79676432736 -05.85684920158 14.3844 13.8893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324205_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 324205_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 324294_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 324294_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 324428_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 324428_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:37:19.22 +00:16:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.358 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324584_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 324584_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 324654_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 324654_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 324765_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 324765_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:49.37 -00:17:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.661 3112668185029745152 105.70514144171 -00.29167765481 14.4099 13.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325055_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 325055_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:03:28.62 +02:05:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.408 3115529079926397440 105.86888862071 +02.08673599505 14.4689 13.8746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325201_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 325201_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 325229_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 325229_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:45:48.03 -05:24:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.883 3100642276602853248 101.44966358979 -05.40758690969 13.9026 12.8468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325274_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 325274_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:43:57.88 +00:24:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.568 3125570816542602880 100.99098774765 +00.40199750005 14.5747 14.1285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.568#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325375_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 325375_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 325429_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 325429_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 325676_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 325676_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 325831_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 325831_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:26.71 -01:47:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.288 3106835550722792576 100.11111020367 -01.80053406046 14.3775 13.7940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325929_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 325929_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:39:22.17 -04:11:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.564 3104000459989380352 099.84229353271 -04.18904210370 14.5055 13.7184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325941_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 325941_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 325994_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 325994_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 326029_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326029_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:02:47.67 -05:24:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.678 3101346616882221440 105.69774484049 -05.41218166336 14.5018 14.0060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326068_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326068_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:57:04.13 -05:29:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.981 3101203508567346304 104.26709385239 -05.49387559270 14.6690 14.2060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326100_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326100_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:04:15.12 -04:59:14.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)
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Considering the candidate 326162_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326162_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:06:57.88 -05:35:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.710 3053324965503140096 106.74095525306 -05.59989769107 14.5506 13.9903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326177_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326177_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 326282_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326282_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:39:46.06 -03:27:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 2.989 3106360492979678336 099.94159449762 -03.45404317783 14.4909 13.7944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326343_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326343_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:24.85 -00:17:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.555 3109712659115220864 107.10346404505 -00.29265099079 14.4327 14.0488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326360_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326360_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:59:43.66 -02:37:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.105 3108906996270577408 104.93142633250 -02.63195994644 14.3673 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326386_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326386_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:40:04.85 -01:42:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 3.396 3106840326726420736 100.02022323952 -01.71588761379 14.7836 14.2312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326461_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326461_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:52:02.23 -02:18:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.380 3106034041105617152 103.00903540639 -02.30088714513 14.6243 14.1363 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 326468_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 326468_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 326490_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 326490_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 326570_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326570_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:08:56.51 -00:19:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.042 3109665070877533952 107.23566746406 -00.32260317632 14.4466 14.0289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326580_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 326580_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:58:24.42 -05:32:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.165 3101006867786907904 104.60159502162 -05.53542119935 14.6855 14.0982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326605_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
Preparing report for the candidate 326605_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
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Considering the candidate 273859_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 273859_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 07:09:13.67 -02:21:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47889_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 47889_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:44:47.62 -05:17:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:41:59.24 -01:11:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:37:53.19 -05:55:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-17_21-39-05_20.00sec_-4.90C_LIGHT_0031 did not pass the final checks
**** FOUND 06:50:00.82 +01:46:34.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 303s
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 ####
06:58:00.73 -02:48:59.5
06:50:09.04 -02:31:58.2
06:55:15.21 -01:21:20.9
06:50:08.07 -01:54:33.7
06:52:48.41 +00:32:44.0
06:53:24.31 -05:41:34.9
07:01:45.78 -05:39:13.9
06:50:09.85 -05:51:27.8
06:55:10.70 -00:02:53.7
07:05:23.22 -03:16:35.0
06:44:26.11 +01:22:07.7
06:57:28.32 -03:51:17.9
06:46:26.60 +00:59:00.9
07:02:13.93 +01:01:50.6
06:56:38.48 -01:07:57.0
07:01:36.94 -04:32:42.4
06:51:10.29 -02:40:55.4
06:53:51.52 -01:16:59.1
06:48:10.24 -01:11:32.8
07:09:00.92 +00:08:34.1
06:49:55.74 +01:56:33.9
07:07:34.51 -03:27:37.5
06:45:12.99 -00:39:26.8
07:09:30.37 -03:52:35.1
06:46:31.23 +01:08:37.5
06:48:15.35 -05:22:24.4
07:05:58.52 -02:49:02.0
06:43:56.53 -05:38:36.8
07:05:19.94 -03:25:10.3
07:01:30.87 -00:10:46.5
06:56:14.48 -03:49:57.5
07:01:52.72 -03:40:33.7
06:47:27.86 -01:05:51.3
06:35:48.88 -05:09:37.2
07:04:23.82 -02:15:17.0
06:50:00.21 -05:55:20.1
06:48:21.40 +01:48:29.4
06:59:42.31 -02:10:52.1
06:52:00.98 +01:29:16.5
06:57:45.68 -04:35:56.6
07:01:23.64 -01:13:44.1
06:57:06.99 -00:31:50.0
06:43:45.87 +00:35:15.8
06:53:08.37 +02:01:28.5
07:09:21.69 +01:07:25.3
06:54:59.11 -05:04:36.6
07:03:39.63 -04:38:24.0
06:53:04.58 -05:33:23.7
06:50:27.80 -05:47:26.4
07:05:05.70 -03:34:36.6
07:03:21.96 -02:28:37.2
06:56:50.41 -06:12:36.7
06:52:41.63 -02:13:43.8
06:49:52.45 -02:39:53.0
07:07:51.45 -05:47:00.2
06:48:31.57 -04:05:32.2
06:46:13.92 +00:50:44.6
06:43:16.57 +00:21:49.1
06:35:07.44 -03:03:04.3
06:57:27.87 -01:45:22.8
07:07:47.25 -05:40:39.1
07:05:04.33 -05:27:54.3
06:58:08.44 -01:38:51.8
06:51:33.01 +00:27:11.8
06:45:12.34 -00:01:52.1
07:06:17.21 +02:00:15.6
06:45:10.86 -03:57:02.9
07:01:50.87 -01:06:59.7
06:43:50.74 +01:35:53.0
07:06:46.03 -06:03:30.4
06:56:22.09 -00:53:11.8
07:08:43.26 -05:05:29.2
06:44:39.63 +00:10:06.6
06:54:48.42 +00:23:17.3
06:42:33.26 -03:28:04.5
06:47:10.34 -05:37:12.5
07:04:16.76 -03:01:37.1
07:06:11.99 +00:18:34.9
06:57:12.45 -03:57:45.1
06:51:18.28 -01:23:08.5
06:49:56.19 -02:40:53.2
06:42:42.23 -01:42:36.1
07:04:56.13 -05:21:47.4
06:54:41.91 -02:41:58.6
06:49:07.27 -01:40:18.2
06:44:57.64 -02:51:43.1
06:48:53.15 +01:49:29.5
06:51:48.81 -04:02:32.3
06:48:57.09 -03:30:58.4
07:04:25.53 -05:07:21.5
06:51:34.25 -01:39:22.9
06:52:36.42 -02:12:53.7
06:46:10.32 -03:13:59.7
07:01:49.55 -05:35:33.2
06:50:41.43 -00:31:44.9
06:49:29.11 -01:29:08.6
06:35:10.35 -00:43:19.3
07:07:03.79 -02:21:52.1
07:03:24.36 -03:02:35.3
06:43:37.03 -04:25:04.2
06:47:15.07 -05:48:25.4
07:08:59.18 -00:34:32.9
06:58:22.49 -02:33:51.6
06:38:41.66 +01:56:37.6
06:45:54.11 -00:09:38.1
06:58:38.36 -00:18:51.2
06:42:30.93 -06:04:22.0
06:52:34.62 +00:32:33.4
07:02:04.11 -01:19:13.0
06:41:27.12 -01:19:00.5
06:49:05.67 -02:35:16.9
06:57:27.66 -05:05:42.4
06:55:15.94 +00:20:59.8
06:53:47.93 +00:29:50.4
06:50:36.89 -01:46:52.9
06:58:20.38 -00:32:39.1
06:54:39.34 +00:12:13.7
06:47:59.57 -01:20:53.8
06:57:35.61 +01:13:54.6
06:49:13.10 -06:00:49.9
06:51:36.55 -02:04:10.2
06:57:11.57 -01:07:45.5
06:49:08.73 -01:39:03.4
06:56:54.15 +00:54:14.4
07:03:54.18 -00:57:00.1
06:48:23.30 -05:30:24.0
06:50:53.26 -04:59:03.0
06:44:11.31 -01:17:52.1
06:51:38.76 -02:45:18.7
06:53:05.91 -05:33:51.7
06:54:01.79 -02:07:17.2
06:59:17.83 -01:38:34.6
06:56:08.05 -03:27:35.8
06:47:53.13 +01:51:22.6
06:47:46.45 -02:22:19.1
06:45:12.42 -00:27:19.8
06:52:51.09 -02:20:52.4
07:06:51.02 -02:07:05.0
06:52:52.61 -00:06:52.1
07:04:10.29 -04:42:09.9
06:52:30.41 -02:40:21.8
06:40:57.66 -03:41:09.5
06:53:47.30 -02:38:44.5
06:49:27.85 -03:07:23.1
06:48:38.26 +01:56:55.9
06:52:15.14 -03:21:31.3
07:09:26.95 -01:59:51.5
06:58:34.76 -01:38:23.6
06:44:26.65 +00:04:54.4
07:01:08.50 -00:12:31.6
06:54:02.99 -00:10:56.6
07:00:46.05 +00:40:10.6
06:40:19.07 +00:02:55.2
07:00:58.84 -04:21:50.3
06:48:25.03 -00:29:08.7
06:46:02.96 +00:29:40.7
07:01:26.07 -05:25:40.3
########### 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 ####
06:58:00.73 -02:48:59.5
06:50:09.04 -02:31:58.2
06:55:15.21 -01:21:20.9
06:50:08.07 -01:54:33.7
06:52:48.41 +00:32:44.0
06:53:24.31 -05:41:34.9
07:01:45.78 -05:39:13.9
06:50:09.85 -05:51:27.8
06:55:10.70 -00:02:53.7
07:05:23.22 -03:16:35.0
06:44:26.11 +01:22:07.7
06:57:28.32 -03:51:17.9
06:46:26.60 +00:59:00.9
07:02:13.93 +01:01:50.6
06:56:38.48 -01:07:57.0
07:01:36.94 -04:32:42.4
06:51:10.29 -02:40:55.4
06:53:51.52 -01:16:59.1
06:48:10.24 -01:11:32.8
07:09:00.92 +00:08:34.1
06:49:55.74 +01:56:33.9
07:07:34.51 -03:27:37.5
06:45:12.99 -00:39:26.8
07:09:30.37 -03:52:35.1
06:46:31.23 +01:08:37.5
06:48:15.35 -05:22:24.4
07:05:58.52 -02:49:02.0
06:43:56.53 -05:38:36.8
07:05:19.94 -03:25:10.3
07:01:30.87 -00:10:46.5
06:56:14.48 -03:49:57.5
07:01:52.72 -03:40:33.7
06:47:27.86 -01:05:51.3
06:35:48.88 -05:09:37.2
07:04:23.82 -02:15:17.0
06:50:00.21 -05:55:20.1
06:48:21.40 +01:48:29.4
06:59:42.31 -02:10:52.1
06:52:00.98 +01:29:16.5
06:57:45.68 -04:35:56.6
07:01:23.64 -01:13:44.1
06:57:06.99 -00:31:50.0
06:43:45.87 +00:35:15.8
06:53:08.37 +02:01:28.5
07:09:21.69 +01:07:25.3
06:54:59.11 -05:04:36.6
07:03:39.63 -04:38:24.0
06:53:04.58 -05:33:23.7
06:50:27.80 -05:47:26.4
07:05:05.70 -03:34:36.6
07:03:21.96 -02:28:37.2
06:56:50.41 -06:12:36.7
06:52:41.63 -02:13:43.8
06:49:52.45 -02:39:53.0
07:07:51.45 -05:47:00.2
06:48:31.57 -04:05:32.2
06:46:13.92 +00:50:44.6
06:43:16.57 +00:21:49.1
06:35:07.44 -03:03:04.3
06:57:27.87 -01:45:22.8
07:07:47.25 -05:40:39.1
07:05:04.33 -05:27:54.3
06:58:08.44 -01:38:51.8
06:51:33.01 +00:27:11.8
06:45:12.34 -00:01:52.1
07:06:17.21 +02:00:15.6
06:45:10.86 -03:57:02.9
07:01:50.87 -01:06:59.7
06:43:50.74 +01:35:53.0
07:06:46.03 -06:03:30.4
06:56:22.09 -00:53:11.8
07:08:43.26 -05:05:29.2
06:44:39.63 +00:10:06.6
06:54:48.42 +00:23:17.3
06:42:33.26 -03:28:04.5
06:47:10.34 -05:37:12.5
07:04:16.76 -03:01:37.1
07:06:11.99 +00:18:34.9
06:57:12.45 -03:57:45.1
06:51:18.28 -01:23:08.5
06:49:56.19 -02:40:53.2
06:42:42.23 -01:42:36.1
07:04:56.13 -05:21:47.4
06:54:41.91 -02:41:58.6
06:49:07.27 -01:40:18.2
06:44:57.64 -02:51:43.1
06:48:53.15 +01:49:29.5
06:51:48.81 -04:02:32.3
06:48:57.09 -03:30:58.4
07:04:25.53 -05:07:21.5
06:51:34.25 -01:39:22.9
06:52:36.42 -02:12:53.7
06:46:10.32 -03:13:59.7
07:01:49.55 -05:35:33.2
06:50:41.43 -00:31:44.9
06:49:29.11 -01:29:08.6
06:35:10.35 -00:43:19.3
07:07:03.79 -02:21:52.1
07:03:24.36 -03:02:35.3
06:43:37.03 -04:25:04.2
06:47:15.07 -05:48:25.4
07:08:59.18 -00:34:32.9
06:58:22.49 -02:33:51.6
06:38:41.66 +01:56:37.6
06:45:54.11 -00:09:38.1
06:58:38.36 -00:18:51.2
06:42:30.93 -06:04:22.0
06:52:34.62 +00:32:33.4
07:02:04.11 -01:19:13.0
06:41:27.12 -01:19:00.5
06:49:05.67 -02:35:16.9
06:57:27.66 -05:05:42.4
06:55:15.94 +00:20:59.8
06:53:47.93 +00:29:50.4
06:50:36.89 -01:46:52.9
06:58:20.38 -00:32:39.1
06:54:39.34 +00:12:13.7
06:47:59.57 -01:20:53.8
06:57:35.61 +01:13:54.6
06:49:13.10 -06:00:49.9
06:51:36.55 -02:04:10.2
06:57:11.57 -01:07:45.5
06:49:08.73 -01:39:03.4
06:56:54.15 +00:54:14.4
07:03:54.18 -00:57:00.1
06:48:23.30 -05:30:24.0
06:50:53.26 -04:59:03.0
06:44:11.31 -01:17:52.1
06:51:38.76 -02:45:18.7
06:53:05.91 -05:33:51.7
06:54:01.79 -02:07:17.2
06:59:17.83 -01:38:34.6
06:56:08.05 -03:27:35.8
06:47:53.13 +01:51:22.6
06:47:46.45 -02:22:19.1
06:45:12.42 -00:27:19.8
06:52:51.09 -02:20:52.4
07:06:51.02 -02:07:05.0
06:52:52.61 -00:06:52.1
07:04:10.29 -04:42:09.9
06:52:30.41 -02:40:21.8
06:40:57.66 -03:41:09.5
06:53:47.30 -02:38:44.5
06:49:27.85 -03:07:23.1
06:48:38.26 +01:56:55.9
06:52:15.14 -03:21:31.3
07:09:26.95 -01:59:51.5
06:58:34.76 -01:38:23.6
06:44:26.65 +00:04:54.4
07:01:08.50 -00:12:31.6
06:54:02.99 -00:10:56.6
07:00:46.05 +00:40:10.6
06:40:19.07 +00:02:55.2
07:00:58.84 -04:21:50.3
06:48:25.03 -00:29:08.7
06:46:02.96 +00:29:40.7
07:01:26.07 -05:25:40.3
###################################################################################
06:58:00.73 -02:48:59.5 -- not an asteroid (will add it to exclusion list)
06:50:09.04 -02:31:58.2 -- not an asteroid (will add it to exclusion list)
06:55:15.21 -01:21:20.9 -- not an asteroid (will add it to exclusion list)
06:50:08.07 -01:54:33.7 -- not an asteroid (will add it to exclusion list)
06:52:48.41 +00:32:44.0 -- not an asteroid (will add it to exclusion list)
06:53:24.31 -05:41:34.9 -- not an asteroid (will add it to exclusion list)
07:01:45.78 -05:39:13.9 -- not an asteroid (will add it to exclusion list)
06:50:09.85 -05:51:27.8 -- not an asteroid (will add it to exclusion list)
06:55:10.70 -00:02:53.7 -- not an asteroid (will add it to exclusion list)
07:05:23.22 -03:16:35.0 -- not an asteroid (will add it to exclusion list)
06:44:26.11 +01:22:07.7 -- not an asteroid (will add it to exclusion list)
06:57:28.32 -03:51:17.9 -- not an asteroid (will add it to exclusion list)
06:46:26.60 +00:59:00.9 -- not an asteroid (will add it to exclusion list)
07:02:13.93 +01:01:50.6 -- not an asteroid (will add it to exclusion list)
06:56:38.48 -01:07:57.0 -- not an asteroid (will add it to exclusion list)
07:01:36.94 -04:32:42.4 -- not an asteroid (will add it to exclusion list)
06:51:10.29 -02:40:55.4 -- not an asteroid (will add it to exclusion list)
06:53:51.52 -01:16:59.1 -- not an asteroid (will add it to exclusion list)
06:48:10.24 -01:11:32.8 -- not an asteroid (will add it to exclusion list)
07:09:00.92 +00:08:34.1 -- not an asteroid (will add it to exclusion list)
06:49:55.74 +01:56:33.9 -- not an asteroid (will add it to exclusion list)
07:07:34.51 -03:27:37.5 -- not an asteroid (will add it to exclusion list)
06:45:12.99 -00:39:26.8 -- not an asteroid (will add it to exclusion list)
07:09:30.37 -03:52:35.1 -- not an asteroid (will add it to exclusion list)
06:46:31.23 +01:08:37.5 -- not an asteroid (will add it to exclusion list)
06:48:15.35 -05:22:24.4 -- not an asteroid (will add it to exclusion list)
07:05:58.52 -02:49:02.0 -- not an asteroid (will add it to exclusion list)
06:43:56.53 -05:38:36.8 -- not an asteroid (will add it to exclusion list)
07:05:19.94 -03:25:10.3 -- not an asteroid (will add it to exclusion list)
07:01:30.87 -00:10:46.5 -- not an asteroid (will add it to exclusion list)
06:56:14.48 -03:49:57.5 -- not an asteroid (will add it to exclusion list)
07:01:52.72 -03:40:33.7 -- not an asteroid (will add it to exclusion list)
06:47:27.86 -01:05:51.3 -- not an asteroid (will add it to exclusion list)
06:35:48.88 -05:09:37.2 -- not an asteroid (will add it to exclusion list)
07:04:23.82 -02:15:17.0 -- not an asteroid (will add it to exclusion list)
06:50:00.21 -05:55:20.1 -- not an asteroid (will add it to exclusion list)
06:48:21.40 +01:48:29.4 -- not an asteroid (will add it to exclusion list)
06:59:42.31 -02:10:52.1 -- not an asteroid (will add it to exclusion list)
06:52:00.98 +01:29:16.5 -- not an asteroid (will add it to exclusion list)
06:57:45.68 -04:35:56.6 -- not an asteroid (will add it to exclusion list)
07:01:23.64 -01:13:44.1 -- not an asteroid (will add it to exclusion list)
06:57:06.99 -00:31:50.0 -- not an asteroid (will add it to exclusion list)
06:43:45.87 +00:35:15.8 -- not an asteroid (will add it to exclusion list)
06:53:08.37 +02:01:28.5 -- not an asteroid (will add it to exclusion list)
07:09:21.69 +01:07:25.3 -- not an asteroid (will add it to exclusion list)
06:54:59.11 -05:04:36.6 -- not an asteroid (will add it to exclusion list)
07:03:39.63 -04:38:24.0 -- not an asteroid (will add it to exclusion list)
06:53:04.58 -05:33:23.7 -- not an asteroid (will add it to exclusion list)
06:50:27.80 -05:47:26.4 -- not an asteroid (will add it to exclusion list)
07:05:05.70 -03:34:36.6 -- not an asteroid (will add it to exclusion list)
07:03:21.96 -02:28:37.2 -- not an asteroid (will add it to exclusion list)
06:56:50.41 -06:12:36.7 -- not an asteroid (will add it to exclusion list)
06:52:41.63 -02:13:43.8 -- not an asteroid (will add it to exclusion list)
06:49:52.45 -02:39:53.0 -- not an asteroid (will add it to exclusion list)
07:07:51.45 -05:47:00.2 -- not an asteroid (will add it to exclusion list)
06:48:31.57 -04:05:32.2 -- not an asteroid (will add it to exclusion list)
06:46:13.92 +00:50:44.6 -- not an asteroid (will add it to exclusion list)
06:43:16.57 +00:21:49.1 -- not an asteroid (will add it to exclusion list)
06:35:07.44 -03:03:04.3 -- not an asteroid (will add it to exclusion list)
06:57:27.87 -01:45:22.8 -- not an asteroid (will add it to exclusion list)
07:07:47.25 -05:40:39.1 -- not an asteroid (will add it to exclusion list)
07:05:04.33 -05:27:54.3 -- not an asteroid (will add it to exclusion list)
06:58:08.44 -01:38:51.8 -- not an asteroid (will add it to exclusion list)
06:51:33.01 +00:27:11.8 -- not an asteroid (will add it to exclusion list)
06:45:12.34 -00:01:52.1 -- not an asteroid (will add it to exclusion list)
07:06:17.21 +02:00:15.6 -- not an asteroid (will add it to exclusion list)
06:45:10.86 -03:57:02.9 -- not an asteroid (will add it to exclusion list)
07:01:50.87 -01:06:59.7 -- not an asteroid (will add it to exclusion list)
06:43:50.74 +01:35:53.0 -- not an asteroid (will add it to exclusion list)
07:06:46.03 -06:03:30.4 -- not an asteroid (will add it to exclusion list)
06:56:22.09 -00:53:11.8 -- not an asteroid (will add it to exclusion list)
07:08:43.26 -05:05:29.2 -- not an asteroid (will add it to exclusion list)
06:44:39.63 +00:10:06.6 -- not an asteroid (will add it to exclusion list)
06:54:48.42 +00:23:17.3 -- not an asteroid (will add it to exclusion list)
06:42:33.26 -03:28:04.5 -- not an asteroid (will add it to exclusion list)
06:47:10.34 -05:37:12.5 -- not an asteroid (will add it to exclusion list)
07:04:16.76 -03:01:37.1 -- not an asteroid (will add it to exclusion list)
07:06:11.99 +00:18:34.9 -- not an asteroid (will add it to exclusion list)
06:57:12.45 -03:57:45.1 -- not an asteroid (will add it to exclusion list)
06:51:18.28 -01:23:08.5 -- not an asteroid (will add it to exclusion list)
06:49:56.19 -02:40:53.2 -- not an asteroid (will add it to exclusion list)
06:42:42.23 -01:42:36.1 -- not an asteroid (will add it to exclusion list)
07:04:56.13 -05:21:47.4 -- not an asteroid (will add it to exclusion list)
06:54:41.91 -02:41:58.6 -- not an asteroid (will add it to exclusion list)
06:49:07.27 -01:40:18.2 -- not an asteroid (will add it to exclusion list)
06:44:57.64 -02:51:43.1 -- not an asteroid (will add it to exclusion list)
06:48:53.15 +01:49:29.5 -- not an asteroid (will add it to exclusion list)
06:51:48.81 -04:02:32.3 -- not an asteroid (will add it to exclusion list)
06:48:57.09 -03:30:58.4 -- not an asteroid (will add it to exclusion list)
07:04:25.53 -05:07:21.5 -- not an asteroid (will add it to exclusion list)
06:51:34.25 -01:39:22.9 -- not an asteroid (will add it to exclusion list)
06:52:36.42 -02:12:53.7 -- not an asteroid (will add it to exclusion list)
06:46:10.32 -03:13:59.7 -- not an asteroid (will add it to exclusion list)
07:01:49.55 -05:35:33.2 -- not an asteroid (will add it to exclusion list)
06:50:41.43 -00:31:44.9 -- not an asteroid (will add it to exclusion list)
06:49:29.11 -01:29:08.6 -- not an asteroid (will add it to exclusion list)
06:35:10.35 -00:43:19.3 -- not an asteroid (will add it to exclusion list)
07:07:03.79 -02:21:52.1 -- not an asteroid (will add it to exclusion list)
07:03:24.36 -03:02:35.3 -- not an asteroid (will add it to exclusion list)
06:43:37.03 -04:25:04.2 -- not an asteroid (will add it to exclusion list)
06:47:15.07 -05:48:25.4 -- not an asteroid (will add it to exclusion list)
07:08:59.18 -00:34:32.9 -- not an asteroid (will add it to exclusion list)
06:58:22.49 -02:33:51.6 -- not an asteroid (will add it to exclusion list)
06:38:41.66 +01:56:37.6 -- not an asteroid (will add it to exclusion list)
06:45:54.11 -00:09:38.1 -- not an asteroid (will add it to exclusion list)
06:58:38.36 -00:18:51.2 -- not an asteroid (will add it to exclusion list)
06:42:30.93 -06:04:22.0 -- not an asteroid (will add it to exclusion list)
06:52:34.62 +00:32:33.4 -- not an asteroid (will add it to exclusion list)
07:02:04.11 -01:19:13.0 -- not an asteroid (will add it to exclusion list)
06:41:27.12 -01:19:00.5 -- not an asteroid (will add it to exclusion list)
06:49:05.67 -02:35:16.9 -- not an asteroid (will add it to exclusion list)
06:57:27.66 -05:05:42.4 -- not an asteroid (will add it to exclusion list)
06:55:15.94 +00:20:59.8 -- not an asteroid (will add it to exclusion list)
06:53:47.93 +00:29:50.4 -- not an asteroid (will add it to exclusion list)
06:50:36.89 -01:46:52.9 -- not an asteroid (will add it to exclusion list)
06:58:20.38 -00:32:39.1 -- not an asteroid (will add it to exclusion list)
06:54:39.34 +00:12:13.7 -- not an asteroid (will add it to exclusion list)
06:47:59.57 -01:20:53.8 -- not an asteroid (will add it to exclusion list)
06:57:35.61 +01:13:54.6 -- not an asteroid (will add it to exclusion list)
06:49:13.10 -06:00:49.9 -- not an asteroid (will add it to exclusion list)
06:51:36.55 -02:04:10.2 -- 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)
06:49:08.73 -01:39:03.4 -- not an asteroid (will add it to exclusion list)
06:56:54.15 +00:54:14.4 -- not an asteroid (will add it to exclusion list)
07:03:54.18 -00:57:00.1 -- not an asteroid (will add it to exclusion list)
06:48:23.30 -05:30:24.0 -- not an asteroid (will add it to exclusion list)
06:50:53.26 -04:59:03.0 -- not an asteroid (will add it to exclusion list)
06:44:11.31 -01:17:52.1 -- not an asteroid (will add it to exclusion list)
06:51:38.76 -02:45:18.7 -- not an asteroid (will add it to exclusion list)
06:53:05.91 -05:33:51.7 -- not an asteroid (will add it to exclusion list)
06:54:01.79 -02:07:17.2 -- not an asteroid (will add it to exclusion list)
06:59:17.83 -01:38:34.6 -- not an asteroid (will add it to exclusion list)
06:56:08.05 -03:27:35.8 -- not an asteroid (will add it to exclusion list)
06:47:53.13 +01:51:22.6 -- not an asteroid (will add it to exclusion list)
06:47:46.45 -02:22:19.1 -- not an asteroid (will add it to exclusion list)
06:45:12.42 -00:27:19.8 -- not an asteroid (will add it to exclusion list)
06:52:51.09 -02:20:52.4 -- not an asteroid (will add it to exclusion list)
07:06:51.02 -02:07:05.0 -- not an asteroid (will add it to exclusion list)
06:52:52.61 -00:06:52.1 -- not an asteroid (will add it to exclusion list)
07:04:10.29 -04:42:09.9 -- not an asteroid (will add it to exclusion list)
06:52:30.41 -02:40:21.8 -- not an asteroid (will add it to exclusion list)
06:40:57.66 -03:41:09.5 -- not an asteroid (will add it to exclusion list)
06:53:47.30 -02:38:44.5 -- not an asteroid (will add it to exclusion list)
06:49:27.85 -03:07:23.1 -- not an asteroid (will add it to exclusion list)
06:48:38.26 +01:56:55.9 -- not an asteroid (will add it to exclusion list)
06:52:15.14 -03:21:31.3 -- not an asteroid (will add it to exclusion list)
07:09:26.95 -01:59:51.5 -- not an asteroid (will add it to exclusion list)
06:58:34.76 -01:38:23.6 -- not an asteroid (will add it to exclusion list)
06:44:26.65 +00:04:54.4 -- not an asteroid (will add it to exclusion list)
07:01:08.50 -00:12:31.6 -- not an asteroid (will add it to exclusion list)
06:54:02.99 -00:10:56.6 -- not an asteroid (will add it to exclusion list)
07:00:46.05 +00:40:10.6 -- not an asteroid (will add it to exclusion list)
06:40:19.07 +00:02:55.2 -- not an asteroid (will add it to exclusion list)
07:00:58.84 -04:21:50.3 -- not an asteroid (will add it to exclusion list)
06:48:25.03 -00:29:08.7 -- not an asteroid (will add it to exclusion list)
06:46:02.96 +00:29:40.7 -- not an asteroid (will add it to exclusion list)
07:01:26.07 -05:25:40.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.44 -03:03:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:10.35 -00:43:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:48.88 -05:09:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:41.66 +01:56:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:19.07 +00:02:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:57.66 -03:41:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.12 -01:19:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:30.93 -06:04:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.26 -03:28:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:42.23 -01:42:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:16.57 +00:21:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:37.03 -04:25:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:45.87 +00:35:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:50.74 +01:35:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:56.53 -05:38:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:11.31 -01:17:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:26.11 +01:22:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:26.65 +00:04:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.63 +00:10:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:57.64 -02:51:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:10.86 -03:57:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.34 -00:01:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.42 -00:27:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.99 -00:39:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:54.11 -00:09:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:02.96 +00:29:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:10.32 -03:13:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.92 +00:50:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:26.60 +00:59:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.23 +01:08:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:10.34 -05:37:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:15.07 -05:48:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:27.86 -01:05:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:46.45 -02:22:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:53.13 +01:51:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.57 -01:20:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:10.24 -01:11:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:15.35 -05:22:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:21.40 +01:48:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:23.30 -05:30:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:25.03 -00:29:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:31.57 -04:05:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:38.26 +01:56:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:53.15 +01:49:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:57.09 -03:30:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:05.67 -02:35:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.27 -01:40:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:08.73 -01:39:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:13.10 -06:00:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:27.85 -03:07:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:29.11 -01:29:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.45 -02:39:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:55.74 +01:56:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.19 -02:40:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:00.21 -05:55:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:08.07 -01:54:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:09.04 -02:31:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:09.85 -05:51:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:27.80 -05:47:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:36.89 -01:46:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.43 -00:31:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:53.26 -04:59:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.29 -02:40:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.28 -01:23:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:33.01 +00:27:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.25 -01:39:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:36.55 -02:04:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:38.76 -02:45:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:48.81 -04:02:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:00.98 +01:29:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:15.14 -03:21:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:30.41 -02:40:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:34.62 +00:32:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:36.42 -02:12:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:41.63 -02:13:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:48.41 +00:32:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:51.09 -02:20:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:52.61 -00:06:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.58 -05:33:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:05.91 -05:33:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:08.37 +02:01:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:24.31 -05:41:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.30 -02:38:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.93 +00:29:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:51.52 -01:16:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:01.79 -02:07:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:02.99 -00:10:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:39.34 +00:12:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.91 -02:41:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.42 +00:23:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:59.11 -05:04:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:10.70 -00:02:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:15.21 -01:21:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:15.94 +00:20:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:08.05 -03:27:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:14.48 -03:49:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.09 -00:53:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:38.48 -01:07:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:50.41 -06:12:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:54.15 +00:54:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:06.99 -00:31:50.0 -- 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)
06:57:12.45 -03:57:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:27.66 -05:05:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:27.87 -01:45:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:28.32 -03:51:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.61 +01:13:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:45.68 -04:35:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:00.73 -02:48:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:08.44 -01:38:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:20.38 -00:32:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:22.49 -02:33:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.76 -01:38:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:38.36 -00:18:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:17.83 -01:38:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:42.31 -02:10:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:46.05 +00:40:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:58.84 -04:21:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:08.50 -00:12:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:23.64 -01:13:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:26.07 -05:25:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:30.87 -00:10:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:36.94 -04:32:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:45.78 -05:39:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:49.55 -05:35:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:50.87 -01:06:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:52.72 -03:40:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:04.11 -01:19:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:13.93 +01:01:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:21.96 -02:28:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.36 -03:02:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:39.63 -04:38:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:54.18 -00:57:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.29 -04:42:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.76 -03:01:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:23.82 -02:15:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:25.53 -05:07:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:56.13 -05:21:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:04.33 -05:27:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:05.70 -03:34:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:19.94 -03:25:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:23.22 -03:16:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:58.52 -02:49:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.99 +00:18:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:17.21 +02:00:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:46.03 -06:03:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:51.02 -02:07:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:03.79 -02:21:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:34.51 -03:27:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:47.25 -05:40:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:51.45 -05:47:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.26 -05:05:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:59.18 -00:34:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:00.92 +00:08:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.69 +01:07:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:26.95 -01:59:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:30.37 -03:52:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:35:07.44 -03:03:04.3 -- not a known variable star
06:35:10.35 -00:43:19.3 -- not a known variable star
06:35:48.88 -05:09:37.2 -- not a known variable star
06:38:41.66 +01:56:37.6 -- not a known variable star
06:40:19.07 +00:02:55.2 -- not a known variable star
06:40:57.66 -03:41:09.5 -- not a known variable star
06:41:27.12 -01:19:00.5 -- a known variable star
06:42:30.93 -06:04:22.0 -- a known variable star
06:42:33.26 -03:28:04.5 -- not a known variable star
06:42:42.23 -01:42:36.1 -- not a known variable star
06:43:16.57 +00:21:49.1 -- a known variable star
06:43:37.03 -04:25:04.2 -- a known variable star
06:43:45.87 +00:35:15.8 -- not a known variable star
06:43:50.74 +01:35:53.0 -- not a known variable star
06:43:56.53 -05:38:36.8 -- a known variable star
06:44:11.31 -01:17:52.1 -- a known variable star
06:44:26.11 +01:22:07.7 -- not a known variable star
06:44:26.65 +00:04:54.4 -- not a known variable star
06:44:39.63 +00:10:06.6 -- a known variable star
06:44:57.64 -02:51:43.1 -- not a known variable star
06:45:10.86 -03:57:02.9 -- not a known variable star
06:45:12.34 -00:01:52.1 -- not a known variable star
06:45:12.42 -00:27:19.8 -- not a known variable star
06:45:12.99 -00:39:26.8 -- not a known variable star
06:45:54.11 -00:09:38.1 -- not a known variable star
06:46:02.96 +00:29:40.7 -- not a known variable star
06:46:10.32 -03:13:59.7 -- a known variable star
06:46:13.92 +00:50:44.6 -- not a known variable star
06:46:26.60 +00:59:00.9 -- not a known variable star
06:46:31.23 +01:08:37.5 -- not a known variable star
06:47:10.34 -05:37:12.5 -- not a known variable star
06:47:15.07 -05:48:25.4 -- not a known variable star
06:47:27.86 -01:05:51.3 -- a known variable star
06:47:46.45 -02:22:19.1 -- not a known variable star
06:47:53.13 +01:51:22.6 -- not a known variable star
06:47:59.57 -01:20:53.8 -- not a known variable star
06:48:10.24 -01:11:32.8 -- a known variable star
06:48:15.35 -05:22:24.4 -- not a known variable star
06:48:21.40 +01:48:29.4 -- not a known variable star
06:48:23.30 -05:30:24.0 -- not a known variable star
06:48:25.03 -00:29:08.7 -- not a known variable star
06:48:31.57 -04:05:32.2 -- a known variable star
06:48:38.26 +01:56:55.9 -- not a known variable star
06:48:53.15 +01:49:29.5 -- a known variable star
06:48:57.09 -03:30:58.4 -- not a known variable star
06:49:05.67 -02:35:16.9 -- not a known variable star
06:49:07.27 -01:40:18.2 -- not a known variable star
06:49:08.73 -01:39:03.4 -- not a known variable star
06:49:13.10 -06:00:49.9 -- a known variable star
06:49:27.85 -03:07:23.1 -- not a known variable star
06:49:29.11 -01:29:08.6 -- not a known variable star
06:49:52.45 -02:39:53.0 -- not a known variable star
06:49:55.74 +01:56:33.9 -- a known variable star
06:49:56.19 -02:40:53.2 -- not a known variable star
06:50:00.21 -05:55:20.1 -- not a known variable star
06:50:08.07 -01:54:33.7 -- not a known variable star
06:50:09.04 -02:31:58.2 -- not a known variable star
06:50:09.85 -05:51:27.8 -- not a known variable star
06:50:27.80 -05:47:26.4 -- not a known variable star
06:50:36.89 -01:46:52.9 -- not a known variable star
06:50:41.43 -00:31:44.9 -- not a known variable star
06:50:53.26 -04:59:03.0 -- not a known variable star
06:51:10.29 -02:40:55.4 -- not a known variable star
06:51:18.28 -01:23:08.5 -- a known variable star
06:51:33.01 +00:27:11.8 -- not a known variable star
06:51:34.25 -01:39:22.9 -- not a known variable star
06:51:36.55 -02:04:10.2 -- a known variable star
06:51:38.76 -02:45:18.7 -- not a known variable star
06:51:48.81 -04:02:32.3 -- a known variable star
06:52:00.98 +01:29:16.5 -- not a known variable star
06:52:15.14 -03:21:31.3 -- not a known variable star
06:52:30.41 -02:40:21.8 -- not a known variable star
06:52:34.62 +00:32:33.4 -- not a known variable star
06:52:36.42 -02:12:53.7 -- not a known variable star
06:52:41.63 -02:13:43.8 -- not a known variable star
06:52:48.41 +00:32:44.0 -- not a known variable star
06:52:51.09 -02:20:52.4 -- not a known variable star
06:52:52.61 -00:06:52.1 -- not a known variable star
06:53:04.58 -05:33:23.7 -- not a known variable star
06:53:05.91 -05:33:51.7 -- a known variable star
06:53:08.37 +02:01:28.5 -- a known variable star
06:53:24.31 -05:41:34.9 -- a known variable star
06:53:47.30 -02:38:44.5 -- not a known variable star
06:53:47.93 +00:29:50.4 -- a known variable star
06:53:51.52 -01:16:59.1 -- not a known variable star
06:54:01.79 -02:07:17.2 -- not a known variable star
06:54:02.99 -00:10:56.6 -- not a known variable star
06:54:39.34 +00:12:13.7 -- not a known variable star
06:54:41.91 -02:41:58.6 -- not a known variable star
06:54:48.42 +00:23:17.3 -- a known variable star
06:54:59.11 -05:04:36.6 -- not a known variable star
06:55:10.70 -00:02:53.7 -- not a known variable star
06:55:15.21 -01:21:20.9 -- a known variable star
06:55:15.94 +00:20:59.8 -- not a known variable star
06:56:08.05 -03:27:35.8 -- a known variable star
06:56:14.48 -03:49:57.5 -- not a known variable star
06:56:22.09 -00:53:11.8 -- a known variable star
06:56:38.48 -01:07:57.0 -- not a known variable star
06:56:50.41 -06:12:36.7 -- not a known variable star
06:56:54.15 +00:54:14.4 -- not a known variable star
06:57:06.99 -00:31:50.0 -- a known variable star
06:57:11.57 -01:07:45.5 -- a known variable star
06:57:12.45 -03:57:45.1 -- not a known variable star
06:57:27.66 -05:05:42.4 -- not a known variable star
06:57:27.87 -01:45:22.8 -- not a known variable star
06:57:28.32 -03:51:17.9 -- not a known variable star
06:57:35.61 +01:13:54.6 -- a known variable star
06:57:45.68 -04:35:56.6 -- a known variable star
06:58:00.73 -02:48:59.5 -- not a known variable star
06:58:08.44 -01:38:51.8 -- not a known variable star
06:58:20.38 -00:32:39.1 -- not a known variable star
06:58:22.49 -02:33:51.6 -- a known variable star
06:58:34.76 -01:38:23.6 -- not a known variable star
06:58:38.36 -00:18:51.2 -- not a known variable star
06:59:17.83 -01:38:34.6 -- not a known variable star
06:59:42.31 -02:10:52.1 -- a known variable star
07:00:46.05 +00:40:10.6 -- not a known variable star
07:00:58.84 -04:21:50.3 -- not a known variable star
07:01:08.50 -00:12:31.6 -- not a known variable star
07:01:23.64 -01:13:44.1 -- not a known variable star
07:01:26.07 -05:25:40.3 -- not a known variable star
07:01:30.87 -00:10:46.5 -- not a known variable star
07:01:36.94 -04:32:42.4 -- not a known variable star
07:01:45.78 -05:39:13.9 -- not a known variable star
07:01:49.55 -05:35:33.2 -- not a known variable star
07:01:50.87 -01:06:59.7 -- not a known variable star
07:01:52.72 -03:40:33.7 -- not a known variable star
07:02:04.11 -01:19:13.0 -- not a known variable star
07:02:13.93 +01:01:50.6 -- a known variable star
07:03:21.96 -02:28:37.2 -- not a known variable star
07:03:24.36 -03:02:35.3 -- not a known variable star
07:03:39.63 -04:38:24.0 -- not a known variable star
07:03:54.18 -00:57:00.1 -- not a known variable star
07:04:10.29 -04:42:09.9 -- not a known variable star
07:04:16.76 -03:01:37.1 -- not a known variable star
07:04:23.82 -02:15:17.0 -- a known variable star
07:04:25.53 -05:07:21.5 -- not a known variable star
07:04:56.13 -05:21:47.4 -- a known variable star
07:05:04.33 -05:27:54.3 -- not a known variable star
07:05:05.70 -03:34:36.6 -- not a known variable star
07:05:19.94 -03:25:10.3 -- a known variable star
07:05:23.22 -03:16:35.0 -- a known variable star
07:05:58.52 -02:49:02.0 -- not a known variable star
07:06:11.99 +00:18:34.9 -- not a known variable star
07:06:17.21 +02:00:15.6 -- not a known variable star
07:06:46.03 -06:03:30.4 -- not a known variable star
07:06:51.02 -02:07:05.0 -- not a known variable star
07:07:03.79 -02:21:52.1 -- not a known variable star
07:07:34.51 -03:27:37.5 -- not a known variable star
07:07:47.25 -05:40:39.1 -- not a known variable star
07:07:51.45 -05:47:00.2 -- a known variable star
07:08:43.26 -05:05:29.2 -- a known variable star
07:08:59.18 -00:34:32.9 -- a known variable star
07:09:00.92 +00:08:34.1 -- a known variable star
07:09:21.69 +01:07:25.3 -- a known variable star
07:09:26.95 -01:59:51.5 -- a known variable star
07:09:30.37 -03:52:35.1 -- a known variable star
Found 114 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
157 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 157 (excluding asteroids and hot pixels, 114 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)2461148.61008652 -observatory V36
00:18:38.81 -00:51:09.6 Mercury (-0.0mag)
03:19:00.28 +18:37:52.4 Venus (-3.9mag)
00:23:49.80 +01:31:23.2 Mars (1.2mag)
07:13:36.80 +22:44:36.4 Jupiter (-2.1mag)
00:30:07.06 +00:54:48.6 Saturn (0.9mag)
03:48:08.71 +19:48:54.6 Uranus (5.8mag)
00:11:06.85 -00:13:38.8 Neptune (7.8mag)
20:33:50.53 -22:52:42.7 Pluto (14.5mag)
02:06:11.76 +17:06:36.4 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 362 Apr 17 21:54 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461148.61008652:
07:13:43.31 +22:44:24.2 Io (5.8mag)
07:13:28.17 +22:44:52.9 Europa (5.9mag)
07:13:23.73 +22:44:58.4 Ganymede (5.4mag)
07:14:03.29 +22:43:35.2 Callisto (6.6mag)
07:16:51.33 +22:31:16.3 Himalia (15.3mag)
07:13:36.19 +22:44:35.5 Thebe (16.2mag)
07:17:05.35 +23:01:34.4 Elara (17.3mag)
07:12:38.30 +23:23:30.5 Pasiphae (17.4mag)
07:21:53.63 +22:42:49.8 Carme (18.5mag)
00:30:00.36 +00:55:15.0 Titan (8.8mag)
00:30:12.18 +00:54:56.1 Rhea (10.1mag)
00:29:43.76 +00:54:37.6 Iapetus (11.5mag)
00:30:07.23 +00:55:16.0 Hyperion (14.8mag)
00:31:42.26 +01:03:22.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 17 21:54 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461148.61008652:
15:47:28.29 -17:40:20.2 JWST
19:13:10.48 +13:42:53.3 Chandra
07:51:26.43 -33:57:55.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 17 21:54 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461148.61008652 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:48.70 -28:54:16.5 13.9mag P/2010 H2 (Vales)
05:08:16.27 -69:33:48.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:54.94 +31:27:07.7 17.2mag C/2017 K2 (PANSTARRS)
17:30:12.15 +10:47:45.7 17.6mag C/2021 G2 (ATLAS)
23:10:45.99 +29:18:50.4 17.1mag C/2022 E2 (ATLAS)
04:31:42.32 +26:05:42.3 16.0mag C/2022 N2 (PANSTARRS)
09:03:54.43 +32:01:37.4 16.2mag C/2022 QE78 (ATLAS)
08:31:25.42 +00:04:02.4 17.3mag C/2022 R6 (PANSTARRS)
18:53:12.11 +18:42:29.2 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:58.33 -11:29:25.9 17.5mag P/2023 B1 (PANSTARRS)
09:06:42.01 -11:32:56.3 17.7mag C/2023 F3 (ATLAS)
21:56:16.47 +63:01:55.8 17.5mag C/2023 H5 (Lemmon)
19:17:17.50 -03:46:12.1 14.1mag C/2023 R1 (PANSTARRS)
21:27:28.64 +86:12:22.4 17.8mag C/2023 X2 (Lemmon)
06:18:57.02 +63:30:20.4 17.2mag C/2024 A1 (ATLAS)
05:17:44.55 +18:59:07.5 11.2mag C/2024 E1 (Wierzchos)
16:17:53.49 +06:44:06.9 17.4mag C/2024 G6 (ATLAS)
20:21:22.02 +15:51:06.8 14.6mag C/2024 J3 (ATLAS)
03:28:16.50 -22:04:02.9 16.3mag C/2024 T5 (ATLAS)
05:18:31.16 +44:46:26.4 17.7mag C/2025 J1 (Borisov)
13:30:07.44 +46:46:21.0 15.3mag C/2025 L1 (ATLAS)
03:28:38.91 -26:32:46.1 17.8mag C/2025 Q3 (ATLAS)
00:05:04.56 +17:40:07.3 8.2mag C/2025 R3 (PANSTARRS)
12:53:12.65 +03:08:19.9 17.4mag C/2025 Y1 (ATLAS)
03:44:04.40 +02:25:06.7 13.9mag C/2026 A1 (MAPS)
00:05:30.10 +37:35:52.7 14.6mag C/2026 B2 (Sun-Gao)
18:47:02.26 -09:36:17.5 11.7mag 10P/Tempel
14:57:26.07 +02:58:54.6 14.2mag 24P/Schaumasse
11:02:15.78 -01:27:35.3 15.7mag 29P/Schwassmann-Wachmann
18:01:29.02 -09:32:04.6 18.0mag 40P/Vaisala
10:37:32.35 -03:56:11.8 16.9mag 43P/Wolf-Harrington
01:51:56.59 +17:50:44.5 17.2mag 47P/Ashbrook-Jackson
07:14:41.96 +36:33:23.8 17.0mag 63P/Wild
23:31:43.80 -11:11:58.1 15.7mag 65P/Gunn
04:08:55.83 +21:58:11.4 15.9mag 76P/West-Kohoutek-Ikemura
01:10:15.17 +08:38:30.4 14.3mag 78P/Gehrels
23:09:20.47 -08:46:00.1 14.6mag 88P/Howell
02:16:24.47 +21:11:54.7 15.1mag 93P/Lovas
04:58:49.28 +32:23:51.1 16.2mag 123P/West-Hartley
08:30:54.81 +37:23:19.3 16.2mag 124P/Mrkos
02:36:29.24 +14:36:13.7 16.4mag 128P/Shoemaker-Holt
02:51:41.04 +14:44:50.5 17.5mag 131P/Mueller
01:37:19.33 +13:56:51.1 10.6mag 141P/Machholz
01:45:56.13 +05:39:45.0 10.6mag 141P-A/Machholz
00:30:15.93 +01:30:15.3 12.6mag 141P-D/Machholz
02:16:24.58 +07:25:16.3 17.8mag 141P-I/Machholz
01:08:16.49 -00:27:43.5 15.0mag 162P/SidingSpring
14:47:41.82 +00:08:25.1 17.7mag 210P/Christensen
21:44:50.90 -10:56:30.9 17.7mag 218P/LINEAR
17:16:59.91 -13:40:39.0 16.1mag 235P/LINEAR
05:39:03.77 +34:51:07.5 16.8mag 240P/NEAT
07:39:33.94 -04:56:34.6 17.7mag 242P/Spahr
22:22:11.07 -20:24:35.5 17.8mag 260P/McNaught
02:02:31.15 +20:59:21.3 18.0mag 295P/LINEAR
15:41:47.59 +07:07:35.5 17.5mag 391P/Kowalski
07:35:02.30 +21:22:15.5 17.7mag 450P/LONEOS
05:38:58.30 +44:54:34.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 17 21:54 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
17:21:59.44 -38:54:04.60 2026-04-14.4 15.15
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
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
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
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
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
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
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
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
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
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
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
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
-rw-r--r-- 1 apache apache 5.8K Apr 17 21:54 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
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
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 17 21:54 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:52:44.230 +56:55:19.06 AT 2026jfc 2026-03-27.87 20.98
14:01:07.200 +03:10:48.03 AT 2026jfb 2026-04-05.73 21.73
13:47:01.080 +02:47:45.39 AT 2026jfa 2026-03-24.91 20.68
17:11:20.724 -17:18:29.68 AT 2026jez 2026-04-04.38 17.507
03:59:36.404 -57:03:28.57 AT 2026jey 2026-04-05.01 18.79
03:57:56.301 -54:05:57.45 AT 2026jex 2026-04-08.01 19.148
10:30:49.649 -08:04:36.38 AT 2026jew 2026-04-07.87 19.144
12:27:21.393 -28:22:09.12 AT 2026jev 2026-04-10.19 18.809
17:40:25.287 +05:08:20.96 AT 2026jeu 2026-04-05.42 17.65
08:35:16.434 -77:00:48.01 AT 2026jet 2026-04-09.11 19.072
21:53:03.051 -16:55:33.84 AT 2026jes 2026-04-10.38 17.345
00:36:19.401 -83:06:05.82 AT 2026jer 2026-04-08.40 18.473
22:08:10.236 -21:46:23.75 AT 2026jeq 2026-04-10.39 18.259
21:34:17.331 -33:37:48.49 AT 2026jep 2026-04-10.39 18.372
16:56:26.248 +04:54:42.94 AT 2026jeo 2026-04-10.42 18.3645
08:10:18.680 +34:40:45.43 AT 2026jen 2026-04-05.17 20.6002
10:14:46.220 +16:03:20.00 AT 2026jem 2026-04-07.20 20.5179
09:08:33.148 +56:28:29.17 AT 2026jel 2026-04-09.15 19.5877
08:06:59.814 +72:49:07.23 AT 2026jek 2026-04-05.15 20.127
10:17:15.279 +45:17:14.78 AT 2026jej 2026-04-08.19 20.2002
-rw-r--r-- 1 apache apache 30K Apr 17 21:54 tns_transients_list.txt
