This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi
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
ZTF J065416.85-003357.2,2461146.6101,13.94,0.05,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
ZTF J065416.85-003357.2 20260416.1101 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461146.6101,13.77,0.05,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 20260416.1101 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,2461146.6101,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1101 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100620904845739776,2461146.6101,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100620904845739776 20260416.1101 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2771-02.2334,2461146.6101,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2771-02.2334 20260416.1101 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107421109384110848,2461146.6101,13.77,0.05,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
Gaia DR3 3107421109384110848 20260416.1101 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,2461146.6101,13.67,0.05,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
target 20260416.1101 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.63,0.05,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 20260416.1101 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
CoRoT 110661942,2461146.6101,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 110661942 20260416.1101 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108804947849328896,2461146.6101,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108804947849328896 20260416.1101 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112170449860484096,2461146.6101,13.71,0.05,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 3112170449860484096 20260416.1101 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
GDS_J0701083-053139,2461146.6101,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0701083-053139 20260416.1101 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8884-03.0051,2461146.6101,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8884-03.0051 20260416.1101 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,2461146.6101,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.6112-02.9740,2461146.6101,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.6112-02.9740 20260416.1101 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.39,0.05,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
target 20260416.1101 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
target,2461146.6101,13.42,0.05,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
target 20260416.1101 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
target,2461146.6101,13.55,0.05,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
target 20260416.1101 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102025152991634560,2461146.6101,13.66,0.05,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 3102025152991634560 20260416.1101 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
Gaia DR3 3108860782423215232,2461146.6101,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108860782423215232 20260416.1101 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.4533-02.0789,2461146.6101,13.41,0.05,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
ATO J104.4533-02.0789 20260416.1101 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,2461146.6101,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107119602680173696,2461146.6101,13.41,0.05,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 3107119602680173696 20260416.1101 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,2461146.6101,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3549-02.2942,2461146.6101,13.55,0.05,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
ATO J107.3549-02.2942 20260416.1101 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3111219166142543104,2461146.6101,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3111219166142543104 20260416.1101 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.1718-00.9990,2461146.6101,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1718-00.9990 20260416.1101 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.44,0.05,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
target 20260416.1101 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.44,0.05,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
target 20260416.1101 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
Gaia DR3 3107583699671179264,2461146.6101,13.38,0.05,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 3107583699671179264 20260416.1101 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,2461146.6101,13.33,0.05,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
target 20260416.1101 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
ATO J101.6375-01.8671,2461146.6101,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.6375-01.8671 20260416.1101 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.33,0.05,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
target 20260416.1101 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
ATO J102.7395-02.0003,2461146.6101,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7395-02.0003 20260416.1101 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9388-05.7085,2461146.6101,13.31,0.05,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
ATO J100.9388-05.7085 20260416.1101 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,2461146.6101,13.41,0.05,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 20260416.1101 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
ATO J101.6222-04.0465,2461146.6101,13.37,0.05,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 J101.6222-04.0465 20260416.1101 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113107165046453504,2461146.6101,13.38,0.05,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 3113107165046453504 20260416.1101 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,2461146.6101,13.45,0.05,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
target 20260416.1101 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9023-03.3839,2461146.6101,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9023-03.3839 20260416.1101 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.31,0.05,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 20260416.1101 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 3106045203719510272,2461146.6101,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106045203719510272 20260416.1101 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.31,0.05,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 20260416.1101 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 3101581706207520000,2461146.6101,13.18,0.05,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 3101581706207520000 20260416.1101 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0207+00.9747,2461146.6101,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0207+00.9747 20260416.1101 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113340978768204672,2461146.6101,13.19,0.05,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
Gaia DR3 3113340978768204672 20260416.1101 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.30,0.05,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 20260416.1101 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 3112536277993759872,2461146.6101,13.22,0.05,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 3112536277993759872 20260416.1101 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
Gaia DR3 3112672888012933248,2461146.6101,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112672888012933248 20260416.1101 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J064630.95+010809.2,2461146.6101,13.40,0.05,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 20260416.1101 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100694159807014016,2461146.6101,13.14,0.05,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
Gaia DR3 3100694159807014016 20260416.1101 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
Gaia DR3 3101629358864500736,2461146.6101,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101629358864500736 20260416.1101 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6668-01.9250,2461146.6101,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6668-01.9250 20260416.1101 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 3053337197571108992,2461146.6101,13.10,0.05,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 3053337197571108992 20260416.1101 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
Gaia DR3 3114737878230131072,2461146.6101,13.09,0.05,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 3114737878230131072 20260416.1101 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 J104.4461+01.4634,2461146.6101,13.04,0.05,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
ATO J104.4461+01.4634 20260416.1101 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,2461146.6101,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9111-04.0918,2461146.6101,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.9111-04.0918 20260416.1101 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 3107712170734171776,2461146.6101,13.06,0.05,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 3107712170734171776 20260416.1101 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.05,0.05,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 20260416.1101 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.99,0.05,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
target 20260416.1101 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 3109005952316009984,2461146.6101,13.07,0.05,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
Gaia DR3 3109005952316009984 20260416.1101 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5329-01.2670,2461146.6101,13.10,0.05,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
ATO J104.5329-01.2670 20260416.1101 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
Gaia DR3 3114460526421262848,2461146.6101,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1101 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3114-06.2236,2461146.6101,12.90,0.05,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
ATO J105.3114-06.2236 20260416.1101 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
ATO J104.4406-02.3939,2461146.6101,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.4406-02.3939 20260416.1101 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108002544877231872,2461146.6101,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108002544877231872 20260416.1101 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
ATO J106.0351+01.0281,2461146.6101,12.91,0.05,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
ATO J106.0351+01.0281 20260416.1101 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 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 3107197805444320128,2461146.6101,12.71,0.05,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 3107197805444320128 20260416.1101 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4191-04.3825,2461146.6101,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4191-04.3825 20260416.1101 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.2634-03.8889,2461146.6101,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.2634-03.8889 20260416.1101 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0457 Mon,2461146.6101,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0457 Mon 20260416.1101 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109500251512786944,2461146.6101,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109500251512786944 20260416.1101 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
V0385 Mon,2461146.6101,12.69,0.05,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
V0385 Mon 20260416.1101 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1974-03.7119,2461146.6101,12.71,0.05,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 J107.1974-03.7119 20260416.1101 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.4640-02.6734,2461146.6101,12.65,0.05,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 J102.4640-02.6734 20260416.1101 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
target,2461146.6101,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109235166132304128,2461146.6101,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109235166132304128 20260416.1101 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102372667384237952,2461146.6101,12.61,0.05,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
Gaia DR3 3102372667384237952 20260416.1101 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.62,0.05,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 20260416.1101 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 3105924742777831040,2461146.6101,12.62,0.05,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
Gaia DR3 3105924742777831040 20260416.1101 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 J104.7374-04.6394,2461146.6101,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7374-04.6394 20260416.1101 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0471-05.0754,2461146.6101,12.56,0.05,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 J106.0471-05.0754 20260416.1101 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
ATO J098.7797-03.0546,2461146.6101,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260416.1101 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125681313161965056,2461146.6101,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125681313161965056 20260416.1101 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.41,0.05,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 20260416.1101 12.41CV 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
ATO J104.7305-03.0153,2461146.6101,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7305-03.0153 20260416.1101 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126780382412815744,2461146.6101,12.07,0.05,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 3126780382412815744 20260416.1101 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 3107234982682679808,2461146.6101,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107234982682679808 20260416.1101 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108867959307360128,2461146.6101,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108867959307360128 20260416.1101 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112130214607270656,2461146.6101,12.07,0.05,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 3112130214607270656 20260416.1101 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 3112151242766551808,2461146.6101,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112151242766551808 20260416.1101 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.9514+00.4118,2461146.6101,11.97,0.05,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 J106.9514+00.4118 20260416.1101 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8986+00.1116,2461146.6101,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.8986+00.1116 20260416.1101 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065134.58+002720.2,2461146.6101,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065134.58+002720.2 20260416.1101 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17210,2461146.6101,9.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 17210 20260416.1101 9.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3075-00.0345,2461146.6101,10.52,0.05,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 J101.3075-00.0345 20260416.1101 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
Gaia DR3 3113144097467624576,2461146.6101,11.05,0.05,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 3113144097467624576 20260416.1101 11.05CV 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 J106.5593+02.0025,2461146.6101,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.5593+02.0025 20260416.1101 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106324999372001664,2461146.6101,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106324999372001664 20260416.1101 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101842737140035712,2461146.6101,12.11,0.05,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 3101842737140035712 20260416.1101 12.11CV 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
ZTF J070631.45-055958.0,2461146.6101,12.27,0.05,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
ZTF J070631.45-055958.0 20260416.1101 12.27CV 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,2461146.6101,12.60,0.05,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
target 20260416.1101 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 3125504223071142784,2461146.6101,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125504223071142784 20260416.1101 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112424230887731712,2461146.6101,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112424230887731712 20260416.1101 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106539296757159680,2461146.6101,12.66,0.05,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 3106539296757159680 20260416.1101 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113610294697190784,2461146.6101,12.66,0.05,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 3113610294697190784 20260416.1101 12.66CV 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
ATO J100.6477-03.4721,2461146.6101,12.71,0.05,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 J100.6477-03.4721 20260416.1101 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6947-02.6960,2461146.6101,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6947-02.6960 20260416.1101 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113732748502887296,2461146.6101,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113732748502887296 20260416.1101 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1101 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112948251257159808,2461146.6101,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112948251257159808 20260416.1101 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 3105921684761121152,2461146.6101,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105921684761121152 20260416.1101 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1101 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105302831513609216,2461146.6101,12.92,0.05,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
Gaia DR3 3105302831513609216 20260416.1101 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 J102.9043-01.6544,2461146.6101,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1101 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101061637209619328,2461146.6101,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101061637209619328 20260416.1101 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 3100657287506385152,2461146.6101,12.91,0.05,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 3100657287506385152 20260416.1101 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 3100691995143597056,2461146.6101,13.03,0.05,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 3100691995143597056 20260416.1101 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
ATO J102.7477+00.2283,2461146.6101,12.97,0.05,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 J102.7477+00.2283 20260416.1101 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 3101401729901835904,2461146.6101,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101401729901835904 20260416.1101 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 3101421727271429888,2461146.6101,12.91,0.05,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 3101421727271429888 20260416.1101 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 3107281540128223104,2461146.6101,13.03,0.05,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 3107281540128223104 20260416.1101 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 3109656416522583808,2461146.6101,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <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 20260416.1101 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102785122,2461146.6101,13.03,0.05,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
CoRoT 102785122 20260416.1101 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 3106831938650976384,2461146.6101,13.07,0.05,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
Gaia DR3 3106831938650976384 20260416.1101 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 3113913996125565440,2461146.6101,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260416.1101 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 3113219246514568576,2461146.6101,13.14,0.05,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
Gaia DR3 3113219246514568576 20260416.1101 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
Gaia DR3 3106128697885405184,2461146.6101,13.05,0.05,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 3106128697885405184 20260416.1101 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 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,2461146.6101,13.10,0.05,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
target 20260416.1101 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9776-05.0786,2461146.6101,13.04,0.05,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
ATO J100.9776-05.0786 20260416.1101 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112636294895145472,2461146.6101,13.09,0.05,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 3112636294895145472 20260416.1101 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 J099.6630+01.9547,2461146.6101,13.12,0.05,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 J099.6630+01.9547 20260416.1101 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,2461146.6101,13.16,0.05,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 20260416.1101 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 3100429448080531584,2461146.6101,13.09,0.05,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 3100429448080531584 20260416.1101 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 3105494249614626944,2461146.6101,13.15,0.05,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 3105494249614626944 20260416.1101 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 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 3125607134785759744,2461146.6101,13.11,0.05,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 3125607134785759744 20260416.1101 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
MGAB-V1272,2461146.6101,13.15,0.05,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
MGAB-V1272 20260416.1101 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 3113342490594252544,2461146.6101,13.15,0.05,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 3113342490594252544 20260416.1101 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 3109541822495218944,2461146.6101,13.11,0.05,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 3109541822495218944 20260416.1101 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 3100441267835993600,2461146.6101,13.14,0.05,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
Gaia DR3 3100441267835993600 20260416.1101 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,2461146.6101,13.10,0.05,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
target 20260416.1101 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
target,2461146.6101,13.29,0.05,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
target 20260416.1101 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
target,2461146.6101,13.20,0.05,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 20260416.1101 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.19,0.05,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
target 20260416.1101 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
ATO J104.1421+00.3123,2461146.6101,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.1421+00.3123 20260416.1101 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3115440431801220224,2461146.6101,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3115440431801220224 20260416.1101 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113700076693885568,2461146.6101,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113700076693885568 20260416.1101 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109309692404188032,2461146.6101,13.22,0.05,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 3109309692404188032 20260416.1101 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
Gaia DR3 3113861047767202048,2461146.6101,13.29,0.05,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 3113861047767202048 20260416.1101 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 J103.1164-04.3756,2461146.6101,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.1164-04.3756 20260416.1101 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113580985840495488,2461146.6101,13.27,0.05,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 3113580985840495488 20260416.1101 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5059+00.7529,2461146.6101,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5059+00.7529 20260416.1101 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2559+00.4104,2461146.6101,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2559+00.4104 20260416.1101 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 3112223325200684160,2461146.6101,13.34,0.05,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 3112223325200684160 20260416.1101 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108863080225629056,2461146.6101,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108863080225629056 20260416.1101 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 3106181925419346432,2461146.6101,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106181925419346432 20260416.1101 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119479006728592256,2461146.6101,13.29,0.05,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 3119479006728592256 20260416.1101 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 3103166854077325312,2461146.6101,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3103166854077325312 20260416.1101 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.29,0.05,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
target 20260416.1101 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 J103.4491-02.6658,2461146.6101,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4491-02.6658 20260416.1101 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8754-05.6870,2461146.6101,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8754-05.6870 20260416.1101 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.9913-01.3476,2461146.6101,13.30,0.05,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
ATO J101.9913-01.3476 20260416.1101 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 3119758209661814272,2461146.6101,13.36,0.05,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 3119758209661814272 20260416.1101 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 3106223840000616320,2461146.6101,13.44,0.05,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 3106223840000616320 20260416.1101 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
Mean magnitude and position on the discovery images:
2026 04 16.1101 2461146.6101 13.53 07:02:14.25 -00:34:58.5
214.68278 2.13656 galactic Mon Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3112609116339522816 | 07:02:14.25 -00:34:58.5 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.768+/-0.030 (K)
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 3112609116339522816,2461146.6101,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3112609116339522816 20260416.1101 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2459-03.9011,2461146.6101,13.37,0.05,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 J103.2459-03.9011 20260416.1101 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 J104.6381-01.6369,2461146.6101,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260416.1101 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8633+01.2636,2461146.6101,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8633+01.2636 20260416.1101 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112311565306916096,2461146.6101,13.41,0.05,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 3112311565306916096 20260416.1101 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
ATO J103.2327-02.3822,2461146.6101,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.2327-02.3822 20260416.1101 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.6630+01.9547,2461146.6101,13.37,0.05,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 J099.6630+01.9547 20260416.1101 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,2461146.6101,13.44,0.05,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
target 20260416.1101 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
Gaia DR3 3106070840385622144,2461146.6101,13.39,0.05,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 3106070840385622144 20260416.1101 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 3104926523657379840,2461146.6101,13.62,0.05,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 3104926523657379840 20260416.1101 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 J105.1271-02.9219,2461146.6101,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.1271-02.9219 20260416.1101 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6381-01.6369,2461146.6101,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260416.1101 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101410934007419008,2461146.6101,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101410934007419008 20260416.1101 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.2067-03.1888,2461146.6101,13.39,0.05,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
ATO J107.2067-03.1888 20260416.1101 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
target,2461146.6101,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0817+01.8035,2461146.6101,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0817+01.8035 20260416.1101 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108873392446804992,2461146.6101,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108873392446804992 20260416.1101 13.76CV 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
target,2461146.6101,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108728497430819456,2461146.6101,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108728497430819456 20260416.1101 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.8630-04.5748,2461146.6101,13.65,0.05,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 J103.8630-04.5748 20260416.1101 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,2461146.6101,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.65,0.05,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 20260416.1101 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
ATO J105.7399-02.5050,2461146.6101,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.7399-02.5050 20260416.1101 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.3694-00.1977,2461146.6101,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.3694-00.1977 20260416.1101 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6381-01.6369,2461146.6101,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260416.1101 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5514-01.0335,2461146.6101,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.5514-01.0335 20260416.1101 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461146.6101,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.76CV 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 3101752748985728512,2461146.6101,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101752748985728512 20260416.1101 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6775-02.8754,2461146.6101,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6775-02.8754 20260416.1101 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106850183672043776,2461146.6101,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106850183672043776 20260416.1101 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9255+01.8510,2461146.6101,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9255+01.8510 20260416.1101 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 3112037443313707264,2461146.6101,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112037443313707264 20260416.1101 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3119613967480138368,2461146.6101,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119613967480138368 20260416.1101 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5858-01.9330,2461146.6101,13.81,0.05,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 J104.5858-01.9330 20260416.1101 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
Gaia DR3 3114572706669550080,2461146.6101,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114572706669550080 20260416.1101 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109701084182004224,2461146.6101,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109701084182004224 20260416.1101 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102339819471535360,2461146.6101,13.78,0.05,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 3102339819471535360 20260416.1101 13.78CV 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 J102.0228+01.8812,2461146.6101,13.77,0.05,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
ATO J102.0228+01.8812 20260416.1101 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
Gaia DR3 3125817485103519104,2461146.6101,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125817485103519104 20260416.1101 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,2461146.6101,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260416.1101 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.2919-01.6972,2461146.6101,13.81,0.05,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 J103.2919-01.6972 20260416.1101 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
target,2461146.6101,13.63,0.05,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 20260416.1101 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 3101069368149567616,2461146.6101,13.77,0.05,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
Gaia DR3 3101069368149567616 20260416.1101 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
Gaia DR3 3111166183426829312,2461146.6101,13.71,0.05,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 3111166183426829312 20260416.1101 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.3369-02.7336,2461146.6101,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.3369-02.7336 20260416.1101 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4394-05.0259,2461146.6101,13.78,0.05,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 J103.4394-05.0259 20260416.1101 13.78CV 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 J105.7560-03.5911,2461146.6101,13.77,0.05,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
ATO J105.7560-03.5911 20260416.1101 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,2461146.6101,13.78,0.05,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
target 20260416.1101 13.78CV 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 3112453054407141504,2461146.6101,13.68,0.05,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
Gaia DR3 3112453054407141504 20260416.1101 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,2461146.6101,13.68,0.05,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 20260416.1101 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 3113779344609660288,2461146.6101,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113779344609660288 20260416.1101 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.6617+00.6472,2461146.6101,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6617+00.6472 20260416.1101 13.93CV 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
target,2461146.6101,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260416.1101 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.8218-02.7605,2461146.6101,13.62,0.05,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
ATO J106.8218-02.7605 20260416.1101 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 J103.8545-02.8955,2461146.6101,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8545-02.8955 20260416.1101 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461146.61038860 16.04.2026 02:38:47.575 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 32244
Objects passed selection criteria: 32120
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: 25968
Average stars matched: 23382.5 (90.0435 %)
Memory usage VmPeak: 132340 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:34:23 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: 2461146.61038860 16.04.2026 02:38:47.575 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 554
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: 234 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): 234849
Objects passed selection criteria: 234021
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: 192183
Average stars matched: 173633 (90.3477 %)
Memory usage VmPeak: 2021096 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:39:49 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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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: 2461146.60977953
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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Image size: 937.3'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: 06:51:31.835 -01:59:55.47 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 06:51:31.835 -01:59:55.47
Angular distance between the image centers 0.0472 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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: 06:51:34.709 -02:00:14.04 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 06:51:34.709 -02:00:14.04
Angular distance between the image centers 0.0349 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:51:31.835 -01:59:55.47
Second-epoch second image center 06:51:34.709 -02:00:14.04
Angular distance between the image centers 0.01303 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.pWQlBribsZ
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.lWgRkJFOAH
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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits &> /tmp/tmp.XZTpTnh4iN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits &> /tmp/tmp.5n2n5r6HTB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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 23 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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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
14.8 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
14.8 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (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.pWQlBribsZ (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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.lWgRkJFOAH (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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.XZTpTnh4iN (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3252, passed=30717
Got 30717 stars (including 27442 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 30717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 30267 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 30266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 30267 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 923 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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.5n2n5r6HTB (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3333, passed=30594
Got 30594 stars (including 27236 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 30594 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 29909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 29909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 29909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58365.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 51883_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 51883_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:20.84 +00:11:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.296 3113354898761323264 103.08687640749 +00.19036365859 12.2558 11.7410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 51884_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 51884_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 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 51892_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 51892_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:36:04.47 -04:43:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 1.067 3103910918510841984 099.01845821580 -04.72563425951 10.7057 9.9795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 51893_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 51893_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:51.25 +00:22:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 2.770 3113516389531142912 102.21376924338 +00.37265378636 11.0074 10.5246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 54179_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 54179_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:13.64 -02:21:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54856_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 54856_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:37.29 -03:49:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56342_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 56342_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:44:58.54 +00:57:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.863 3125630563829023488 101.24400728112 +00.95149061823 11.6686 11.2387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 57002_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57002_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:09.63 -02:35:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.641 3105917355433930880 102.79000853321 -02.59546837364 11.5920 10.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57102_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57102_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:23.85 -02:23:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.976 3106155498479577600 101.59922268247 -02.39400212671 11.9676 11.5712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57195_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57195_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:44:47.53 -05:17:45.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57390_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57390_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:45.31 +00:41:48.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57581_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57581_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:24.47 -02:50:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57651_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57651_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:36.15 -02:12:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.250 3106608119313089792 100.65078624539 -02.20722417901 11.9774 11.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57661_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57661_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:44.21 -02:34:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.418 3106104714788050432 101.93458736101 -02.57691600924 12.0161 11.7182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57797_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57797_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:23.78 -02:34:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57817_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57817_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:43:57.72 -05:05:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.689 3100715669003273088 100.99050597606 -05.08366354313 11.8817 11.3420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57973_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 57973_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:56:06.78 -01:13:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.917 3112127873846137728 104.02800960912 -01.23330860926 11.8306 11.0479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58159_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 58159_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:53.16 +01:21:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.828 3126065214517150080 102.72155493317 +01.36552187352 12.3588 11.9139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58186_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 58186_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:37:55.83 -01:31:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58191_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 58191_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:09.69 -00:09:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.398 3112904988045623936 104.54016124858 -00.15649212873 12.1035 11.6459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58267_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 58267_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:43.82 -01:42:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.162 3106312659922857984 102.18249398242 -01.70133781615 12.0350 11.7576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58274_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 58274_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:50.22 -05:33:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.397 3101894379828642944 102.95915856284 -05.56087713298 11.9962 11.6123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58365_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 58365_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:50.05 -02:30:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 2.542 3106150722477720192 101.70886789962 -02.50965411492 11.8322 11.0362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Image size: 937.3'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: 06:51:31.835 -01:59:55.47 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 06:51:31.835 -01:59:55.47
Angular distance between the image centers 0.0472 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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: 06:51:34.709 -02:00:14.04 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 06:51:34.709 -02:00:14.04
Angular distance between the image centers 0.0349 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 06:51:31.835 -01:59:55.47
Second-epoch second image center 06:51:34.709 -02:00:14.04
Angular distance between the image centers 0.01303 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.hIoRF1Czen
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.3fh6G3DNO7
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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits &> /tmp/tmp.mkdHkYQ3Q1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits &> /tmp/tmp.G5gNonK2C0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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 464 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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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
14.1 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
14.1 mag. fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
All-image limiting magnitude estimate: 14.1 (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.hIoRF1Czen (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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.3fh6G3DNO7 (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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.mkdHkYQ3Q1 (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=68, blended=33158, passed=206735
Got 206735 stars (including 173367 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 206735 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 201391 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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 201389 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 201392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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.G5gNonK2C0 (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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=75, blended=33918, passed=210230
Got 210230 stars (including 176065 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 210230 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 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(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 204486 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 -7.3 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: 930 matched stars entering correct_measured_positions(), 204485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 204481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 930 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_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/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_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-37-54_20.00sec_-4.90C_LIGHT_0037.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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_2026-04-15_CI_Mon-02-Q2b1x1_222848_TTUQ2b1x1_20310_evlsIvyi/wcs_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038.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
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
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
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
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
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
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out283635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283656.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out322204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out326892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329649.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out283729.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out283757.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out283817.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out283930.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out283975.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out284011.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out312900.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out326290.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out328080.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out328738.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out283654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283837.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283885.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out287148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out299583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304866.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312193.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312714.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314546.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out326539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out327994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329209.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329774.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 292s
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: 141s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283635_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283635_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:02.91 -04:50:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.448 3059440998933764224 107.01117331229 -04.84254210889 14.4141 13.9439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283649_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:18.06 -00:22:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 5.383 3113217425448537856 102.32504394673 -00.38375868588 14.8798 14.4128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283654_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283654_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283655_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283655_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283656_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283656_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:04:13.87 -01:45:12.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)
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Considering the candidate 283659_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283659_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283681_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283681_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283685_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283685_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 283686_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283686_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:57:59.45 -02:49:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.376 3102904899732941696 104.49714302472 -02.81813202334 14.5928 14.0513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283688_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283688_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:56:54.36 -05:54:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 5.334 3100964880188054400 104.22577093736 -05.91265332590 14.4914 13.4668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283699_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283699_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:36:36.57 +00:54:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.626 3120598756240844928 099.15166320957 +00.91237451295 14.1954 13.4200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283701_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283701_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:22.51 -05:32:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.244 3053340599185309824 107.09300747588 -05.54396697811 14.2908 14.0677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283707_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283707_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283710_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283710_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:04:58.02 -03:31:14.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 283712_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283712_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283713_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283713_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 283717_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283717_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:20.80 -03:32:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.031 3107719214480432384 107.08606179048 -03.54738744885 14.3221 13.8907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283723_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:18.19 +00:22:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.639 3113375583324359552 103.57504988742 +00.36559261201 14.3411 13.4385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283726_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283726_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:47.01 -00:06:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.033 3112864344776363264 104.69554828933 -00.11623812816 14.5861 13.7118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283727_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283727_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:57:45.72 -00:25:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.570 3112474911501474560 104.43977838691 -00.43062480543 14.8311 14.2604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283728_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283728_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283729_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283729_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:25.53 -01:37:04.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 283731_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283731_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283733_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283733_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283739_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283739_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 283746_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283746_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:04.92 +00:16:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.376 3113556418627340160 102.52022265106 +00.27669937215 14.2226 13.2762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283748_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283748_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283754_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283754_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283757_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283757_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:02.95 -01:16:43.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 283759_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283759_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283763_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283763_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:24.50 -03:13:58.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
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Considering the candidate 283768_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283768_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:59.85 -00:21:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.296 3112663473446184960 105.49907785949 -00.35692531128 14.2894 13.4175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283776_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283776_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:57:58.93 -03:42:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.728 3102632220849897856 104.49479038638 -03.71010329575 14.3280 13.8617 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 283779_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283779_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:29.95 -03:52:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.249 3107647265186583808 107.37374359299 -03.87668655923 14.3528 13.8822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283783_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283783_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283787_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283787_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283800_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283800_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:41.73 -03:32:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.824 3105572418019801216 100.67337610879 -03.54957724967 14.2149 13.4973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283806_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283806_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:23.69 +01:30:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.811 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283815_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283815_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283816_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283816_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283817_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283817_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:33.91 -02:02:21.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 283829_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283829_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283837_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283837_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283838_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283838_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283845_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283845_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:55:15.89 +01:54:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.489 3114197605703190144 103.81594044377 +01.91519884715 14.5763 14.0033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283847_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283847_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:55.58 -06:11:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.190 3052869698970583168 105.48124573053 -06.20015329687 14.1228 13.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283852_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:20.83 -00:17:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.069 3107460343905382912 101.58623755812 -00.28548509265 14.2042 13.5171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283855_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283855_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283856_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283856_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:48.18 +00:48:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.234 3113780031804890240 103.70024235816 +00.80414763310 14.2644 13.5974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283869_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283869_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283874_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283874_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283875_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283875_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:45.97 +01:43:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.033 3114190768115468544 103.44074071667 +01.72916096446 14.2925 13.7012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283883_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283883_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:14.65 -05:48:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283884_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283884_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283885_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283885_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283886_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283886_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:13.35 +00:50:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.454 3125567827244921728 101.55524044974 +00.83678768778 13.7948 12.7251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283888_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283888_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283902_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283902_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283903_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283903_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:05.92 -05:33:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.967 3101146368322338688 103.27432865352 -05.56475238862 14.4088 13.9864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283906_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283906_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 283909_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283909_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283911_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283911_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283914_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283914_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283918_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:17.15 -04:56:00.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 283919_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283919_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:39.28 -00:11:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 5.147 3113246871743868672 102.66307355868 -00.20118987143 14.2112 13.6471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283920_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283920_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283924_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283924_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:19.12 -01:02:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 4.038 3109413218295766400 107.32904768222 -01.03529667759 14.0534 13.5389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283926_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283926_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283927_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283927_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:24.33 -05:42:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.541 3053146054344208768 107.35077537873 -05.71427999805 14.0854 13.3733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283930_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283930_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:01.86 -03:10:13.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 283934_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283934_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283935_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283935_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283939_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283939_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283940_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283940_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283944_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283944_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283947_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283947_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:31.08 +01:58:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.666 3126161975841384064 102.37858773006 +01.96593928574 14.2878 13.4320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283949_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283949_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283954_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283954_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283961_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283961_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283964_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283964_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 283967_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283967_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:43.72 -02:26:01.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 283971_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283971_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283975_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283975_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:47.47 -00:37:50.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 283978_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283978_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283981_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283981_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:00:26.27 -01:14:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.445 3112171583731862912 105.10955329640 -01.24825779821 14.0990 13.4064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283982_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:00:39.20 -01:30:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.723 3109160601198102528 105.16357336797 -01.50895654099 13.8323 13.0787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283987_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283987_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:06:51.41 -02:03:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.817 3109196820665249664 106.71366696630 -02.06464853213 14.0010 13.7456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283989_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 283989_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:27.17 -05:35:51.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 283992_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 283992_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284002_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284002_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:51.93 +00:01:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.115 3113451445327095424 102.21594845509 +00.02355261831 13.8506 13.3312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284004_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284004_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 284006_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284006_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284011_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284011_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:01.36 -00:36:15.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 284023_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284023_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:30.99 -05:49:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.367 3053120765576879104 107.12881578633 -05.82463316389 14.0753 13.5372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284027_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284027_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:43:04.69 +01:03:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.937 3125820714918979840 100.76924916467 +01.05284958449 13.7488 12.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284032_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284032_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:44.98 -03:41:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.654 3107703821317850368 107.43704622586 -03.69891737982 13.8124 13.3638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284034_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284034_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:03:20.30 +01:33:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.517 3115401055542013568 105.83420033145 +01.55585162026 13.8464 12.8763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284035_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284035_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284037_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284037_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284039_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284039_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284041_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284041_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284042_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284042_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:03:39.86 -04:38:24.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 284045_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284045_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284046_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284046_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:47.04 +01:14:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.263 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284049_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284049_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284055_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284055_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284056_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284056_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284057_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284057_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:57.08 +00:43:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.737 3125594799639377024 100.73738555000 +00.73187374331 13.4606 12.4772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284063_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284063_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284064_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284064_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:43:11.76 -02:02:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.756 3106617259003491456 100.79850991076 -02.03450460142 13.7064 13.1691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284066_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284066_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:06:50.43 +00:50:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 284069_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284069_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284073_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284073_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:25.40 -03:36:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.066 3107820060307074816 106.35605107274 -03.60946233271 13.9552 13.1959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284074_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284074_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:17.83 +02:11:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.086 3126792202162858240 100.57392687056 +02.18444643850 13.9378 13.4510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284082_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284082_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284084_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284084_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284089_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284089_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284090_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284090_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:05.73 -03:34:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.514 3107823290122505600 106.27336488213 -03.57763826488 13.9752 13.7154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284092_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284092_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284094_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284094_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284095_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284095_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:53.00 -01:58:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.165 3106817065184077312 100.22043042317 -01.97855920489 13.6217 13.0149 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 284097_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284097_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284099_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284099_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:19.40 -01:29:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.232 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284100_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284100_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 284102_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284102_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:06.58 +00:28:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.541 3113392007278549888 103.27695675982 +00.46879719149 13.5732 13.0519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284103_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284103_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:06.26 -04:00:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.799 3107769203592227584 106.27515859253 -04.00446217511 13.6174 13.0843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284108_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284108_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:04.47 -05:53:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.308 3101108259073557760 103.01829861414 -05.88727505251 13.5348 13.0509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284109_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284109_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:37.59 -02:21:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 5.445 3106690204730551936 099.65602265592 -02.35585984284 13.2484 12.1574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284111_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284111_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284113_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284113_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:23.86 -05:15:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.606 3101964366313335296 102.59896228734 -05.26153723479 13.5496 13.0347 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 284119_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284119_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284126_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284126_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284127_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284127_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284128_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284128_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:25.47 +02:12:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.087 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284131_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284131_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284134_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284134_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284142_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284142_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284146_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284146_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284147_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284147_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:06:33.49 -02:33:38.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284150_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284150_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:49.54 -04:00:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 4.146 3107586688968496896 106.45583434320 -04.00474451455 13.5009 13.1766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284152_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284152_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284153_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284153_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284155_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284155_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:43.54 +01:59:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.301 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284156_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284156_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:34:57.65 -03:16:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 2.647 3105103235793238656 098.73981880354 -03.26962395126 13.2415 12.6962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284160_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284160_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284163_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284163_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:43:52.87 +01:17:51.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284164_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284164_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284165_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284165_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284166_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284166_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:14.17 +02:01:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.856 3126352844188307968 102.05855649241 +02.02585059891 12.8269 11.8611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284167_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284167_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284169_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284169_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:25.55 -02:40:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.030 3108912390749031168 104.60594672572 -02.67627969568 13.3638 13.0142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284171_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284171_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:12.76 +00:51:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284174_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284174_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284177_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284177_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284182_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284182_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:56.09 -05:49:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284186_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284186_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284188_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284188_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:46.82 -05:40:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 2.725 3053314279624776064 106.94456846585 -05.68169598615 12.9995 12.8098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284190_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284190_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:50.14 -01:53:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 5.252 3109030828766502528 104.70977051143 -01.88815536144 13.1130 12.4796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284192_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284192_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284193_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284193_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:04.29 -05:27:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 2.628 3053295381770283008 106.26741413958 -05.46587345470 13.1606 12.4833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284196_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284196_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:02.47 +01:07:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284200_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284200_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:08.24 -05:53:00.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284201_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284201_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284202_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284202_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284205_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284205_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284206_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284206_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:54.64 +00:53:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284207_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284207_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284210_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284210_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284212_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284212_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284216_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284216_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:50.75 +01:53:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284221_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284221_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:57:09.52 -00:01:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.365 3112923061267990016 104.28919243697 -00.01964918706 12.2320 11.4108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284222_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284222_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:35.68 +01:46:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284223_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284223_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:11.77 -01:33:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284225_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284225_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284229_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 284229_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:45:59.04 -04:51:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.95, MAG_FAINT_SEARCH_LIMIT=11.93)GAIADR2_OUTPUT=# 1.023 3102224366453166976 101.49580560879 -04.86373564501 11.8140 11.5763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284231_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 284231_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 287144_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 287144_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:40.20 -00:32:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 287148_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 287148_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 287577_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 287577_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:01.62 -00:05:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 1.944 3112865238129521920 104.75657781092 -00.08934525517 11.1791 10.2020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288808_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 288808_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:37.27 +00:27:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289272_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 289272_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289437_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 289437_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:39.77 +00:25:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 289740_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 289740_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:37.77 +00:43:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 290896_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 290896_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:30.63 -01:04:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291360_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 291360_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:04:10.75 -03:14:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 291766_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 291766_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:11.30 -06:02:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292072_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 292072_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:41.64 -00:33:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 292952_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 292952_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:57:39.92 -05:17:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 1.893 3101213777831416960 104.41613637585 -05.29032131842 12.4704 11.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293273_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 293273_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296767_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 296767_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:31.30 +00:46:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 3.619 3114351331172456192 106.87951415988 +00.76727923449 12.7081 11.6609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 297254_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 297254_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:44.58 -04:35:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 298507_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 298507_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299583_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 299583_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299639_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 299639_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:45:00.25 -00:03:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 299651_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 299651_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:03.44 -02:29:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 3.238 3108405756407264640 107.26382902829 -02.48563387066 13.1420 12.7775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300106_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 300106_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301406_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 301406_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:34:15.03 -05:19:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.523 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301512_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 301512_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:45:04.81 -01:02:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.772 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302032_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 302032_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:54.34 +00:00:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.714 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302158_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 302158_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:13.69 +01:34:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.815 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302924_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 302924_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:17.59 -04:25:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.768 3103981287255761536 100.07307980311 -04.43283226625 13.2340 12.7718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303121_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 303121_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:22.53 -03:06:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 303501_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 303501_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:17.70 -03:14:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.291 3108624696661653888 105.57310754703 -03.24292917899 13.4515 12.7613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304548_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 304548_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304866_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 304866_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305114_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 305114_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:07.48 -01:52:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 305357_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 305357_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:43:50.78 +01:35:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 5.208 3125993196509475712 100.96104386401 +01.59687974744 13.5411 13.0702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305569_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 305569_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306120_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 306120_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306474_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 306474_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:55.15 -02:23:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.191 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307026_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 307026_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307232_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 307232_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:14.85 -02:18:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 4.983 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307297_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 307297_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307585_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 307585_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:14.08 -00:06:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 3.906 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307591_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 307591_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:44:26.26 -06:06:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.037 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307646_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 307646_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:23.46 -01:36:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.825 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308363_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 308363_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308641_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 308641_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:41:18.61 -00:51:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.076 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308856_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 308856_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308917_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 308917_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309238_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 309238_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309792_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 309792_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309891_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 309891_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309956_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 309956_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:56:43.22 +02:11:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 310880_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 310880_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:10.15 -04:14:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.739 3102354765961077376 102.29138349722 -04.24606660808 13.4027 12.2461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311018_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311018_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:41:47.08 -00:16:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.696 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311159_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311159_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:33.42 +01:51:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311379_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311379_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:21.06 -03:11:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.003 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311396_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311396_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:05.37 -04:41:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.663 3103780042268573568 100.02241043894 -04.69454432899 13.8502 13.0386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311410_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311410_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:46.58 -02:44:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.494 3106508927049985280 100.69338451398 -02.73839649824 13.7626 13.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311451_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 311451_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311495_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311495_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:10.40 -01:01:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.985 3112567987734134144 105.29366963077 -01.02124268361 13.7541 13.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311553_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 311553_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311590_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311590_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:20.59 -00:31:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311802_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 311802_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:00:53.43 +02:12:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.675 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312145_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 312145_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:29.74 -04:08:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.014 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312150_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 312150_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312193_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 312193_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312248_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 312248_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:26.38 -02:20:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.555 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312508_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 312508_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:41:05.55 -05:41:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 4.590 3100575683127182848 100.27197276181 -05.68650192790 13.9287 13.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312714_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 312714_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312900_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 312900_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:26.83 -02:55:48.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313006_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 313006_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313051_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 313051_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:20.42 -05:15:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.201 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313191_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 313191_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313268_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 313268_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313449_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 313449_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313620_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 313620_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:36:32.44 -03:35:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.215 3104844850559457792 099.13443358317 -03.59975014338 14.0155 13.4377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313681_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 313681_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:04:24.76 -04:44:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.571 3101515254479426176 106.10305967209 -04.74501396050 13.8733 13.4014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313794_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 313794_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313848_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 313848_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313860_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 313860_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:48.81 -04:02:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.949 3102343049290484992 102.95330842454 -04.04267620034 13.9995 13.2065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313942_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 313942_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:04.14 +01:58:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 314071_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 314071_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314079_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 314079_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314290_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 314290_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314536_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 314536_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:53.23 +01:49:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.342 3126153111029053568 102.22144351024 +01.82425048629 13.8939 13.4215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314546_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 314546_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314627_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 314627_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315139_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 315139_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315344_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 315344_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:55:12.56 +01:46:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 315440_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 315440_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:01.08 -00:33:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.320 3112656021682569600 105.50481814040 -00.56507854051 13.8943 13.0707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315520_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 315520_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 315605_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 315605_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:27.35 -05:52:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.900 3101108916207784960 103.11340523708 -05.87976646569 14.0840 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315746_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 315746_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:25.94 -01:49:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.604 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315747_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 315747_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 315791_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 315791_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 315888_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 315888_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 316024_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316024_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:39:08.70 -03:48:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.815 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316309_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 316309_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 316315_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316315_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:26.06 -05:48:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 316316_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 316316_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 316422_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316422_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:37:33.28 +01:24:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 4.218 3120687370005889280 099.38804092931 +01.40995382945 13.9336 13.3825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316448_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316448_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:06:14.87 -04:55:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.177 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316515_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316515_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:52.49 +01:12:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.772 3120620024919006848 099.71870063274 +01.20611895865 14.1237 13.6672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316522_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316522_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:49.47 +00:27:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 3.386 3114279519319862400 107.20543385668 +00.45405634620 13.8903 13.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 316952_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 316952_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:03:39.64 -00:16:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.773 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317125_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 317125_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:42:31.03 -06:04:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.149 3100477590376003456 100.62876710199 -06.07316657315 14.0485 13.2618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317407_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 317407_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 317452_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 317452_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 317508_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 317508_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:09.67 -05:17:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.254 3100639871420927872 101.78975441255 -05.28971896782 13.7735 12.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 317890_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 317890_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318041_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318041_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318050_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 318050_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:26.00 -04:02:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.663 3107548171700995200 107.35768740344 -04.04303758020 14.0826 13.5872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318218_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318218_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318318_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318318_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318374_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318374_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318376_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 318376_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:40.21 -00:26:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.124 3112511367183611136 103.66730236160 -00.44919517720 13.9757 13.1957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318383_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318383_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318830_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318830_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318842_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 318842_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:45.83 -03:24:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.507 3102672387384334464 104.94054368107 -03.40607048421 14.1574 13.6542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318874_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 318874_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 318936_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 318936_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:14.78 -03:39:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.348 3105452708691209216 101.81087051013 -03.65148798860 13.4646 12.2211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319032_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319032_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319050_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 319050_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:22.45 +01:18:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.854 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 319257_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319257_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319352_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319352_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319365_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319365_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319434_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319434_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319464_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319464_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319496_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319496_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319788_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 319788_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:06:54.26 +02:10:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 319809_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319809_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 319830_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 319830_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 320160_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 320160_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 320397_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 320397_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:57.64 -02:12:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.885 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320641_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 320641_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 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 320723_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 320723_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:38.13 -00:17:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.501 3119433956814456704 099.65819127034 -00.29763616830 14.2367 13.6075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320731_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 320731_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:47.97 +00:29:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.348 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 320846_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 320846_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 321059_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 321059_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 321151_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 321151_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:19.51 +00:10:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 4.655 3113463028857506944 102.33095298829 +00.17350196522 14.2638 13.4483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321273_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 321273_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:02.74 -00:42:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.268 3109627588701789184 106.76082783589 -00.70808447428 14.2295 13.7367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321454_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 321454_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:37.08 -01:46:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.186 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321652_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 321652_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 321655_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 321655_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:38.91 +00:36:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.013 3113619949783427072 102.41144535065 +00.61020120759 13.8962 12.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321656_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 321656_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 321740_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 321740_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:48:44.05 -05:54:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.223 3100366264824580480 102.18279250022 -05.90788495291 13.4790 12.3244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321800_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 321800_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 322019_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 322019_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:27.76 +01:39:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 3.573 3126135209605384448 102.36549196435 +01.66385619264 14.1154 13.6175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322034_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 322034_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:53.50 -00:49:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.805 3119330641377186688 099.72224575617 -00.82187219144 14.2480 13.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322191_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 322191_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:42.55 +00:17:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.867 3112951201897467136 104.92679471042 +00.29040761527 14.3636 13.5626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322204_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 322204_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:33.98 -00:46:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.489 3112262774476682112 104.89085647506 -00.77602993535 14.3279 13.8367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322456_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 322456_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 322655_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 322655_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 322785_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 322785_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 322802_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 322802_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 322863_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 322863_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:28.79 -01:01:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.251 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322870_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 322870_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 323001_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 323001_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 323539_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 323539_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 323550_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 323550_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 323614_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 323614_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:18.30 -02:07:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.631 3106051805090685696 103.57553630608 -02.12473732458 14.3576 13.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323690_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 323690_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:49.38 -00:17:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.911 3112668185029745152 105.70514144171 -00.29167765481 14.4099 13.7294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323805_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 323805_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 323836_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 323836_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 323996_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 323996_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:42.28 -04:00:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.032 3102564085489488640 104.67532896095 -04.00403705487 14.3505 13.8415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324062_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 324062_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 324074_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 324074_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 324105_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 324105_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:02.95 +01:17:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 5.335 3114067687234902528 103.26150189626 +01.29007914832 14.2536 13.7674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324232_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 324232_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:33:29.02 +01:58:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.079 3120965610869943424 098.36990336847 +01.97793607089 13.8185 12.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324585_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 324585_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:00.91 -02:29:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.607 3108405378450160640 107.25314373552 -02.49393719618 14.0537 13.2542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324591_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 324591_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324834_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 324834_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:40:26.84 -01:47:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.913 3106835550722792576 100.11111020367 -01.80053406046 14.3775 13.7940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324841_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 324841_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 324967_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 324967_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:45:24.59 -02:02:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.009 3106935846799955712 101.35189817049 -02.04941269651 14.3338 13.8621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325054_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 325054_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:05.59 +00:51:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.412 3113605484332811648 103.02252679260 +00.85637243039 14.3468 13.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325177_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 325177_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 325428_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 325428_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 325461_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 325461_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:12.14 -06:01:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 325577_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 325577_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:29.68 -05:31:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.498 3053331322044768768 106.87363336958 -05.52963771220 14.1610 13.5036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325658_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 325658_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 325747_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 325747_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 325776_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 325776_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:46:39.62 -05:23:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.378 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325979_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 325979_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 326176_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326176_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:55:46.76 -02:13:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.842 3111993291050240640 103.94412015801 -02.21882222783 14.3688 13.7456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326223_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 326223_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 326256_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326256_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:08.63 -00:01:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.792 3111232837019910656 107.03525090547 -00.03362767301 14.2683 13.7055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326290_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326290_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:55:11.87 +00:56:25.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 326326_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326326_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:55:08.62 -05:32:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.130 3101224399288448640 103.78562300676 -05.53637445239 14.1525 13.0830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326343_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326343_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:18.87 -03:53:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.410 3107609744353600384 106.82769021894 -03.89510999930 14.5073 14.0244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326467_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326467_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:37.31 -02:20:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.280 3106690380827599744 099.65466382938 -02.33500260524 14.3936 13.7053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326532_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326532_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:51:10.20 -02:47:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.164 3105909590133909760 102.79168393796 -02.80018181706 14.4805 14.0038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326539_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 326539_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 326661_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326661_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:00:18.29 -02:50:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.935 3108711450697385728 105.07587775535 -02.84123636943 14.5976 14.2292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 326892_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 326892_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:03:28.66 +02:05:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.425 3115529079926397440 105.86888862071 +02.08673599505 14.4689 13.8746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327096_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327096_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:14.59 -03:03:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.637 3105876261188224384 102.56025388385 -03.05058131472 14.1551 13.1411 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 327102_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327102_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327112_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327112_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:24.91 -00:17:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.264 3109712659115220864 107.10346404505 -00.29265099079 14.4327 14.0488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327240_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327240_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327242_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327242_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327379_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327379_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327430_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327430_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327592_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327592_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:39.76 -05:32:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.689 3101322943021932416 105.41473552941 -05.53560980801 14.4739 14.0037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327612_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327612_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:43.67 -02:37:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.484 3108906996270577408 104.93142633250 -02.63195994644 14.3673 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327656_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327656_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327673_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327673_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327705_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327705_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:24.50 -01:03:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.957 3107126508988092544 102.35130968936 -01.05111434072 14.5931 13.8441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327745_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327745_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327780_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327780_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327805_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327805_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:33.55 +02:09:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.236 3126238460618897792 103.63897544738 +02.16303910243 14.5450 13.9446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327910_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327910_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 327947_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 327947_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:27.10 -05:07:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.680 3101407193100020864 105.61222071183 -05.12908457613 14.5026 13.9552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 327969_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327969_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 327994_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 327994_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 328080_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328080_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:31.54 +01:42:08.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)
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Considering the candidate 328107_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328107_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 328201_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328201_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 328257_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328257_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
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Considering the candidate 328333_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328333_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:52.14 +00:49:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 5.272 3113659944517871104 102.46656884662 +00.83187008901 14.3851 13.8439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328351_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328351_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328354_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328354_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328408_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328408_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328414_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328414_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328442_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328442_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328494_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328494_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328502_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328502_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328507_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328507_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328625_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328625_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:05.77 -01:36:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.158 3106285485671334784 103.02345645078 -01.60554724780 14.5023 13.6142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328678_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328678_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328690_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328690_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:03:31.90 -04:48:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 4.087 3101515941674339968 105.88221958335 -04.81734233597 14.4205 13.9643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328709_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328709_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:12.09 -02:20:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 4.544 3108997293662134400 104.79962658383 -02.33451681197 14.6167 14.2326 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328714_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328714_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:33:54.22 -00:01:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.694 3119680698390201344 098.47500551942 -00.02182169194 14.1106 13.0776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328738_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328738_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:23.56 -05:11:39.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328764_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328764_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:05:40.07 -05:52:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.243 3053225322262390656 106.41637127690 -05.87441269746 14.6240 14.2104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328836_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328836_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:47:02.71 +01:28:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.916 3125764158789355008 101.76083209082 +01.47509741618 14.5520 13.9921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328906_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328906_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:17.80 -05:11:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.552 3053411586406203264 106.82354465304 -05.18990697635 14.6259 14.0440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 328922_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328922_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:06:38.97 -01:53:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.169 3109252895757025920 106.66172268544 -01.88689027584 14.4879 13.9728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328937_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328937_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:00.29 -01:14:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 4.580 3112162787639018112 104.75077684722 -01.24658584771 14.7511 14.3696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328954_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328954_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:56:47.39 +00:29:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.074 3113730072741558272 104.19687239559 +00.49405138811 14.6154 13.8350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328960_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 328960_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:00:46.04 -00:47:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.662 3112623135114648960 105.19109279001 -00.79374862002 14.2400 13.2249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 328996_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 328996_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329010_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329010_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329048_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329048_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329108_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329108_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:49:49.00 -05:55:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.867 3100357090774324864 102.45354244608 -05.92770976357 14.6224 14.0637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329121_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329121_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:09.12 -04:07:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.884 3107534152928192512 107.28726652518 -04.13143194844 14.3172 14.0151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329134_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329134_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329135_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329135_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:03:44.04 -04:39:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.968 3101531609714913536 105.93276972588 -04.65113314865 14.5382 13.9983 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329140_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329140_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:59:27.41 +01:42:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 4.217 3115454450574501632 104.86391953538 +01.71411472969 14.6770 14.2260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329146_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329146_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329161_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329161_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329204_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329204_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329209_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329209_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329212_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329212_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329236_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329236_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:38:51.74 -00:42:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.967 3119338097440359808 099.71524006389 -00.71388818350 14.7763 14.1758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329299_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329299_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329344_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329344_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:04:35.36 -02:55:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.934 3108751518456730240 106.14659876532 -02.92747671806 14.4783 13.9795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329345_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329345_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:15.75 -02:47:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.168 3105943331397415168 103.31515666666 -02.79302299532 14.8140 14.3458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329351_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329351_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329362_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329362_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:37:19.34 +00:16:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.850 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329382_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329382_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:52.22 -02:37:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.625 3105971334584697216 103.71669581737 -02.62504076135 13.9313 12.7828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329406_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329406_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329446_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329446_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329492_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329492_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:54:34.44 -01:09:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.226 3112325648499548032 103.64279549227 -01.15626921023 14.5400 13.9947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329497_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329497_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:04:28.78 -00:46:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.496 3109591029940494720 106.11895183041 -00.77137633199 14.7889 14.2134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329505_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329505_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329515_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329515_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:02:33.65 -01:05:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.773 3109550382370294912 105.64051879278 -01.09356612467 14.6414 14.0611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329563_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329563_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:53:45.38 +01:59:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.177 3126206162465063296 103.43878066168 +01.99257415158 14.6770 14.1324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329610_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329610_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:07:04.96 -03:43:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.056 3107621422360979328 106.76982168879 -03.72520651955 14.4877 13.9565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329617_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329617_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329640_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329640_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329649_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329649_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:52:51.78 -03:30:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.780 3102785293483602816 103.21521802092 -03.51676705530 14.5044 13.5733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329659_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329659_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329774_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
Preparing report for the candidate 329774_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329810_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329810_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:58:44.92 -02:12:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.384 3109002752559773184 104.68691826078 -02.21644699691 14.8326 14.2518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 329815_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 329815_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:01:48.28 -05:16:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.916 3101398568805887616 105.45051131308 -05.28389797131 14.6740 14.1755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:50:00.86 +01:46:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:09:13.69 -02:21:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 07:08:45.36 +00:41:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-15_21-38-47_20.00sec_-5.00C_LIGHT_0038 did not pass the final checks
**** FOUND 06:37:53.22 -05:55:13.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 11s
make_report_in_HTML.sh TOTAL: 444s
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 ####
06:54:17.53 -00:33:49.3
06:59:05.20 -00:46:04.2
06:54:25.07 -05:50:48.5
06:44:56.02 -05:29:00.7
06:57:07.03 -02:14:45.0
06:42:37.07 +00:51:08.7
06:43:28.37 -00:41:03.8
06:52:48.53 +00:32:44.3
06:59:50.28 -01:50:12.9
06:50:08.87 -05:03:54.2
07:05:29.09 -02:26:14.4
07:00:42.70 -01:17:01.4
07:01:08.52 -05:31:36.8
06:59:33.19 -02:59:48.1
06:44:49.26 +00:56:55.9
06:50:27.41 -02:58:41.8
06:43:35.56 +02:06:58.4
07:01:16.54 -02:28:43.2
06:45:11.99 +00:14:17.9
07:07:34.54 -03:27:34.5
06:53:34.00 -04:54:50.0
07:04:23.82 -02:15:16.5
06:57:48.02 -02:04:24.0
07:05:16.10 -05:50:54.2
06:48:10.30 -01:11:30.7
06:45:13.10 -00:39:25.7
07:09:24.60 -02:17:49.3
07:08:16.87 -00:08:18.0
07:00:43.17 -00:59:23.0
06:50:18.59 -02:39:12.6
06:43:14.44 +01:58:18.5
07:06:42.72 -04:01:01.9
07:03:37.03 -00:12:38.1
06:46:32.65 -01:51:12.9
06:58:42.27 -06:03:35.1
06:50:57.46 -01:59:56.3
06:43:46.58 -05:42:06.3
06:58:43.39 -01:49:10.8
06:46:28.56 -04:02:41.2
07:02:14.16 +01:01:53.4
07:06:05.17 -02:24:58.8
07:03:36.19 -03:22:58.6
06:52:38.64 -04:12:06.4
06:53:52.25 -02:12:22.6
06:54:05.49 -01:51:47.4
06:59:51.28 -05:11:53.9
07:04:05.71 +00:58:06.3
06:52:37.15 +00:04:33.8
07:01:30.96 -00:10:45.7
06:55:40.74 -00:18:33.6
07:02:32.47 -00:13:09.9
06:46:31.34 +01:08:38.7
06:45:14.20 -05:17:04.5
06:59:55.77 -04:44:52.9
06:58:39.28 -01:55:23.7
07:09:13.77 -05:35:54.4
07:05:46.02 +01:40:01.9
06:57:47.56 +01:28:14.8
06:52:01.09 +01:29:17.6
06:47:38.70 -04:05:19.3
07:09:31.23 -03:28:28.4
07:02:23.80 -01:34:40.9
06:53:04.60 -05:33:22.4
06:59:42.37 -02:10:52.6
06:58:08.98 -01:15:49.1
07:09:21.66 +01:07:25.9
07:01:15.32 -06:13:19.2
06:57:44.29 -02:24:17.8
07:05:20.07 -02:51:44.0
07:04:08.37 +01:01:41.5
07:03:33.58 -05:00:26.0
06:48:07.73 -00:40:38.5
07:09:41.24 -04:22:45.0
07:05:04.14 -03:53:19.4
06:56:56.53 -01:54:46.4
07:07:09.42 -01:15:16.5
07:09:10.76 -05:50:44.5
07:08:48.66 -03:42:58.5
06:49:52.64 -02:41:00.1
07:07:57.09 -00:27:58.3
07:09:08.56 -01:41:28.2
06:48:31.66 -04:05:32.3
06:46:14.00 +00:50:44.4
06:49:52.45 -02:39:52.4
06:58:59.35 -04:37:56.1
07:04:10.27 -05:04:54.6
06:35:07.45 -03:03:03.8
07:02:17.23 -03:49:24.0
06:49:22.99 +01:06:39.9
06:49:46.88 -00:33:12.0
06:58:57.13 -03:00:40.6
06:42:58.68 +02:07:38.8
06:41:45.21 -01:18:56.8
07:05:51.00 -02:05:12.1
06:59:00.75 -01:39:59.9
06:57:47.67 -01:31:05.7
07:07:48.17 +00:24:44.0
06:59:36.62 +00:07:20.8
06:51:33.07 +00:27:12.9
06:51:43.99 +00:27:50.8
06:45:12.38 -00:01:52.0
06:50:14.56 -00:47:11.7
07:06:17.18 +02:00:15.7
06:51:05.02 -01:41:33.3
07:00:51.52 -03:52:02.8
07:06:30.20 -06:00:00.2
07:01:48.98 +01:06:04.3
06:44:39.70 +00:10:07.3
06:56:22.11 -00:53:11.0
06:43:08.74 -02:33:59.4
06:48:48.76 +00:23:22.6
06:42:33.25 -03:28:04.7
06:54:43.83 -02:41:21.8
06:57:07.90 +00:36:03.3
06:49:07.41 -01:40:17.5
06:59:43.81 +00:17:13.3
06:49:56.12 -02:40:53.6
06:42:42.28 -01:42:35.9
06:43:36.97 -04:25:01.2
06:51:34.34 -01:39:23.3
06:55:24.49 -05:54:31.1
06:46:12.68 -05:08:48.1
06:43:44.34 -05:07:45.9
06:50:59.53 +00:13:39.6
07:01:28.13 -05:15:07.2
07:01:22.85 -05:01:11.0
06:41:27.04 -01:19:01.9
07:08:59.19 -00:34:32.2
06:45:33.74 -00:26:16.5
06:41:21.26 -01:43:18.6
06:57:35.85 +01:13:54.0
06:50:41.51 -00:31:43.8
06:49:56.12 -02:17:03.1
06:54:17.85 -04:54:46.6
06:48:57.08 -03:30:57.5
06:43:55.57 -05:04:00.5
07:01:15.48 -00:32:58.4
06:38:41.64 +01:56:39.6
07:05:35.96 -05:43:55.9
06:47:15.17 -05:48:24.0
06:48:34.70 -03:13:29.3
06:57:27.90 -05:05:42.5
06:45:17.66 +00:43:38.6
07:05:00.39 -01:12:33.6
06:51:28.50 -00:06:28.4
07:03:46.90 -01:04:50.9
06:48:23.31 -05:30:24.5
06:53:13.94 -04:35:48.9
06:47:44.87 +00:19:24.7
06:49:24.69 -00:56:16.7
06:58:20.47 -00:32:37.7
06:56:35.74 +00:19:16.8
07:00:15.99 +01:37:06.2
06:55:15.98 +00:20:60.0
07:07:24.04 -01:20:23.1
07:01:19.02 +01:03:48.3
06:52:28.75 -04:22:31.2
06:52:34.77 +00:32:34.7
06:50:01.96 +00:45:50.3
06:56:58.64 +00:23:51.1
06:57:11.64 -01:07:43.9
07:04:51.63 -02:12:04.3
06:47:46.59 -02:22:19.2
06:41:55.53 -00:07:52.6
06:38:28.93 -06:01:35.0
06:44:20.03 +01:40:51.7
06:53:47.32 -02:38:43.9
07:07:30.06 -05:41:17.4
06:47:59.64 -01:20:54.3
06:39:41.58 +00:27:18.9
06:50:45.39 -02:12:09.1
07:02:14.25 -00:34:58.5
07:00:01.85 -04:09:56.7
06:52:59.53 -03:53:49.7
06:58:34.20 -01:38:07.0
07:07:29.55 +01:15:33.2
06:55:00.90 -01:15:39.7
06:52:56.39 -02:22:52.9
06:38:39.62 +01:56:42.4
06:59:11.07 -01:18:50.5
06:53:59.16 -01:54:56.0
06:37:40.99 -03:18:48.9
07:00:30.86 -02:55:26.7
06:58:34.80 -01:38:24.4
07:02:16.89 -05:05:04.7
07:08:50.18 -03:10:51.0
06:49:52.53 +01:17:48.6
07:00:20.22 +01:48:28.5
07:05:23.70 -01:58:45.1
06:45:19.63 +01:14:09.9
07:02:16.17 -02:43:01.8
06:55:28.08 -04:33:51.7
06:56:38.66 -01:07:55.9
07:04:55.72 -05:17:03.6
07:02:58.20 -02:30:17.1
06:45:26.17 -00:11:49.7
07:02:25.77 -04:08:33.5
06:58:30.33 -01:38:04.9
06:58:09.49 -01:01:48.7
06:47:15.19 +00:57:18.3
07:03:41.18 -04:17:19.7
06:54:43.78 -02:51:58.3
06:40:44.67 -01:31:43.2
06:59:41.69 +01:51:43.3
06:57:56.90 -01:46:47.0
06:36:38.18 -00:15:15.0
06:58:19.61 -01:55:23.3
07:06:38.71 +01:16:42.5
07:07:45.52 -00:30:37.7
06:52:06.83 -04:04:30.1
06:48:03.89 +01:52:53.7
06:43:53.86 +01:01:55.1
07:02:45.55 -04:03:43.9
06:53:09.57 -01:41:52.7
06:55:30.26 -05:25:59.0
06:54:15.66 -05:56:34.7
07:09:08.15 -00:17:49.6
06:53:19.90 -02:43:44.0
06:53:47.66 -05:01:30.8
07:03:04.29 -03:35:09.1
07:06:17.21 -01:42:55.2
06:57:35.00 -00:39:10.9
07:06:11.24 -01:44:21.0
06:54:20.75 +00:46:57.4
06:54:38.30 +00:38:49.8
06:55:22.13 -00:31:19.0
07:07:15.26 -02:45:45.9
06:55:22.82 -02:54:14.1
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:54:17.53 -00:33:49.3
06:59:05.20 -00:46:04.2
06:54:25.07 -05:50:48.5
06:44:56.02 -05:29:00.7
06:57:07.03 -02:14:45.0
06:42:37.07 +00:51:08.7
06:43:28.37 -00:41:03.8
06:52:48.53 +00:32:44.3
06:59:50.28 -01:50:12.9
06:50:08.87 -05:03:54.2
07:05:29.09 -02:26:14.4
07:00:42.70 -01:17:01.4
07:01:08.52 -05:31:36.8
06:59:33.19 -02:59:48.1
06:44:49.26 +00:56:55.9
06:50:27.41 -02:58:41.8
06:43:35.56 +02:06:58.4
07:01:16.54 -02:28:43.2
06:45:11.99 +00:14:17.9
07:07:34.54 -03:27:34.5
06:53:34.00 -04:54:50.0
07:04:23.82 -02:15:16.5
06:57:48.02 -02:04:24.0
07:05:16.10 -05:50:54.2
06:48:10.30 -01:11:30.7
06:45:13.10 -00:39:25.7
07:09:24.60 -02:17:49.3
07:08:16.87 -00:08:18.0
07:00:43.17 -00:59:23.0
06:50:18.59 -02:39:12.6
06:43:14.44 +01:58:18.5
07:06:42.72 -04:01:01.9
07:03:37.03 -00:12:38.1
06:46:32.65 -01:51:12.9
06:58:42.27 -06:03:35.1
06:50:57.46 -01:59:56.3
06:43:46.58 -05:42:06.3
06:58:43.39 -01:49:10.8
06:46:28.56 -04:02:41.2
07:02:14.16 +01:01:53.4
07:06:05.17 -02:24:58.8
07:03:36.19 -03:22:58.6
06:52:38.64 -04:12:06.4
06:53:52.25 -02:12:22.6
06:54:05.49 -01:51:47.4
06:59:51.28 -05:11:53.9
07:04:05.71 +00:58:06.3
06:52:37.15 +00:04:33.8
07:01:30.96 -00:10:45.7
06:55:40.74 -00:18:33.6
07:02:32.47 -00:13:09.9
06:46:31.34 +01:08:38.7
06:45:14.20 -05:17:04.5
06:59:55.77 -04:44:52.9
06:58:39.28 -01:55:23.7
07:09:13.77 -05:35:54.4
07:05:46.02 +01:40:01.9
06:57:47.56 +01:28:14.8
06:52:01.09 +01:29:17.6
06:47:38.70 -04:05:19.3
07:09:31.23 -03:28:28.4
07:02:23.80 -01:34:40.9
06:53:04.60 -05:33:22.4
06:59:42.37 -02:10:52.6
06:58:08.98 -01:15:49.1
07:09:21.66 +01:07:25.9
07:01:15.32 -06:13:19.2
06:57:44.29 -02:24:17.8
07:05:20.07 -02:51:44.0
07:04:08.37 +01:01:41.5
07:03:33.58 -05:00:26.0
06:48:07.73 -00:40:38.5
07:09:41.24 -04:22:45.0
07:05:04.14 -03:53:19.4
06:56:56.53 -01:54:46.4
07:07:09.42 -01:15:16.5
07:09:10.76 -05:50:44.5
07:08:48.66 -03:42:58.5
06:49:52.64 -02:41:00.1
07:07:57.09 -00:27:58.3
07:09:08.56 -01:41:28.2
06:48:31.66 -04:05:32.3
06:46:14.00 +00:50:44.4
06:49:52.45 -02:39:52.4
06:58:59.35 -04:37:56.1
07:04:10.27 -05:04:54.6
06:35:07.45 -03:03:03.8
07:02:17.23 -03:49:24.0
06:49:22.99 +01:06:39.9
06:49:46.88 -00:33:12.0
06:58:57.13 -03:00:40.6
06:42:58.68 +02:07:38.8
06:41:45.21 -01:18:56.8
07:05:51.00 -02:05:12.1
06:59:00.75 -01:39:59.9
06:57:47.67 -01:31:05.7
07:07:48.17 +00:24:44.0
06:59:36.62 +00:07:20.8
06:51:33.07 +00:27:12.9
06:51:43.99 +00:27:50.8
06:45:12.38 -00:01:52.0
06:50:14.56 -00:47:11.7
07:06:17.18 +02:00:15.7
06:51:05.02 -01:41:33.3
07:00:51.52 -03:52:02.8
07:06:30.20 -06:00:00.2
07:01:48.98 +01:06:04.3
06:44:39.70 +00:10:07.3
06:56:22.11 -00:53:11.0
06:43:08.74 -02:33:59.4
06:48:48.76 +00:23:22.6
06:42:33.25 -03:28:04.7
06:54:43.83 -02:41:21.8
06:57:07.90 +00:36:03.3
06:49:07.41 -01:40:17.5
06:59:43.81 +00:17:13.3
06:49:56.12 -02:40:53.6
06:42:42.28 -01:42:35.9
06:43:36.97 -04:25:01.2
06:51:34.34 -01:39:23.3
06:55:24.49 -05:54:31.1
06:46:12.68 -05:08:48.1
06:43:44.34 -05:07:45.9
06:50:59.53 +00:13:39.6
07:01:28.13 -05:15:07.2
07:01:22.85 -05:01:11.0
06:41:27.04 -01:19:01.9
07:08:59.19 -00:34:32.2
06:45:33.74 -00:26:16.5
06:41:21.26 -01:43:18.6
06:57:35.85 +01:13:54.0
06:50:41.51 -00:31:43.8
06:49:56.12 -02:17:03.1
06:54:17.85 -04:54:46.6
06:48:57.08 -03:30:57.5
06:43:55.57 -05:04:00.5
07:01:15.48 -00:32:58.4
06:38:41.64 +01:56:39.6
07:05:35.96 -05:43:55.9
06:47:15.17 -05:48:24.0
06:48:34.70 -03:13:29.3
06:57:27.90 -05:05:42.5
06:45:17.66 +00:43:38.6
07:05:00.39 -01:12:33.6
06:51:28.50 -00:06:28.4
07:03:46.90 -01:04:50.9
06:48:23.31 -05:30:24.5
06:53:13.94 -04:35:48.9
06:47:44.87 +00:19:24.7
06:49:24.69 -00:56:16.7
06:58:20.47 -00:32:37.7
06:56:35.74 +00:19:16.8
07:00:15.99 +01:37:06.2
06:55:15.98 +00:20:60.0
07:07:24.04 -01:20:23.1
07:01:19.02 +01:03:48.3
06:52:28.75 -04:22:31.2
06:52:34.77 +00:32:34.7
06:50:01.96 +00:45:50.3
06:56:58.64 +00:23:51.1
06:57:11.64 -01:07:43.9
07:04:51.63 -02:12:04.3
06:47:46.59 -02:22:19.2
06:41:55.53 -00:07:52.6
06:38:28.93 -06:01:35.0
06:44:20.03 +01:40:51.7
06:53:47.32 -02:38:43.9
07:07:30.06 -05:41:17.4
06:47:59.64 -01:20:54.3
06:39:41.58 +00:27:18.9
06:50:45.39 -02:12:09.1
07:02:14.25 -00:34:58.5
07:00:01.85 -04:09:56.7
06:52:59.53 -03:53:49.7
06:58:34.20 -01:38:07.0
07:07:29.55 +01:15:33.2
06:55:00.90 -01:15:39.7
06:52:56.39 -02:22:52.9
06:38:39.62 +01:56:42.4
06:59:11.07 -01:18:50.5
06:53:59.16 -01:54:56.0
06:37:40.99 -03:18:48.9
07:00:30.86 -02:55:26.7
06:58:34.80 -01:38:24.4
07:02:16.89 -05:05:04.7
07:08:50.18 -03:10:51.0
06:49:52.53 +01:17:48.6
07:00:20.22 +01:48:28.5
07:05:23.70 -01:58:45.1
06:45:19.63 +01:14:09.9
07:02:16.17 -02:43:01.8
06:55:28.08 -04:33:51.7
06:56:38.66 -01:07:55.9
07:04:55.72 -05:17:03.6
07:02:58.20 -02:30:17.1
06:45:26.17 -00:11:49.7
07:02:25.77 -04:08:33.5
06:58:30.33 -01:38:04.9
06:58:09.49 -01:01:48.7
06:47:15.19 +00:57:18.3
07:03:41.18 -04:17:19.7
06:54:43.78 -02:51:58.3
06:40:44.67 -01:31:43.2
06:59:41.69 +01:51:43.3
06:57:56.90 -01:46:47.0
06:36:38.18 -00:15:15.0
06:58:19.61 -01:55:23.3
07:06:38.71 +01:16:42.5
07:07:45.52 -00:30:37.7
06:52:06.83 -04:04:30.1
06:48:03.89 +01:52:53.7
06:43:53.86 +01:01:55.1
07:02:45.55 -04:03:43.9
06:53:09.57 -01:41:52.7
06:55:30.26 -05:25:59.0
06:54:15.66 -05:56:34.7
07:09:08.15 -00:17:49.6
06:53:19.90 -02:43:44.0
06:53:47.66 -05:01:30.8
07:03:04.29 -03:35:09.1
07:06:17.21 -01:42:55.2
06:57:35.00 -00:39:10.9
07:06:11.24 -01:44:21.0
06:54:20.75 +00:46:57.4
06:54:38.30 +00:38:49.8
06:55:22.13 -00:31:19.0
07:07:15.26 -02:45:45.9
06:55:22.82 -02:54:14.1
###################################################################################
06:54:17.53 -00:33:49.3 -- not an asteroid (will add it to exclusion list)
06:59:05.20 -00:46:04.2 -- not an asteroid (will add it to exclusion list)
06:54:25.07 -05:50:48.5 -- not an asteroid (will add it to exclusion list)
06:44:56.02 -05:29:00.7 -- not an asteroid (will add it to exclusion list)
06:57:07.03 -02:14:45.0 -- not an asteroid (will add it to exclusion list)
06:42:37.07 +00:51:08.7 -- not an asteroid (will add it to exclusion list)
06:43:28.37 -00:41:03.8 -- not an asteroid (will add it to exclusion list)
06:52:48.53 +00:32:44.3 -- not an asteroid (will add it to exclusion list)
06:59:50.28 -01:50:12.9 -- not an asteroid (will add it to exclusion list)
06:50:08.87 -05:03:54.2 -- not an asteroid (will add it to exclusion list)
07:05:29.09 -02:26:14.4 -- not an asteroid (will add it to exclusion list)
07:00:42.70 -01:17:01.4 -- not an asteroid (will add it to exclusion list)
07:01:08.52 -05:31:36.8 -- not an asteroid (will add it to exclusion list)
06:59:33.19 -02:59:48.1 -- not an asteroid (will add it to exclusion list)
06:44:49.26 +00:56:55.9 -- not an asteroid (will add it to exclusion list)
06:50:27.41 -02:58:41.8 -- not an asteroid (will add it to exclusion list)
06:43:35.56 +02:06:58.4 -- not an asteroid (will add it to exclusion list)
07:01:16.54 -02:28:43.2 -- not an asteroid (will add it to exclusion list)
06:45:11.99 +00:14:17.9 -- not an asteroid (will add it to exclusion list)
07:07:34.54 -03:27:34.5 -- not an asteroid (will add it to exclusion list)
06:53:34.00 -04:54:50.0 -- not an asteroid (will add it to exclusion list)
07:04:23.82 -02:15:16.5 -- not an asteroid (will add it to exclusion list)
06:57:48.02 -02:04:24.0 -- not an asteroid (will add it to exclusion list)
07:05:16.10 -05:50:54.2 -- not an asteroid (will add it to exclusion list)
06:48:10.30 -01:11:30.7 -- not an asteroid (will add it to exclusion list)
06:45:13.10 -00:39:25.7 -- not an asteroid (will add it to exclusion list)
07:09:24.60 -02:17:49.3 -- not an asteroid (will add it to exclusion list)
07:08:16.87 -00:08:18.0 -- not an asteroid (will add it to exclusion list)
07:00:43.17 -00:59:23.0 -- not an asteroid (will add it to exclusion list)
06:50:18.59 -02:39:12.6 -- not an asteroid (will add it to exclusion list)
06:43:14.44 +01:58:18.5 -- not an asteroid (will add it to exclusion list)
07:06:42.72 -04:01:01.9 -- not an asteroid (will add it to exclusion list)
07:03:37.03 -00:12:38.1 -- not an asteroid (will add it to exclusion list)
06:46:32.65 -01:51:12.9 -- not an asteroid (will add it to exclusion list)
06:58:42.27 -06:03:35.1 -- not an asteroid (will add it to exclusion list)
06:50:57.46 -01:59:56.3 -- not an asteroid (will add it to exclusion list)
06:43:46.58 -05:42:06.3 -- not an asteroid (will add it to exclusion list)
06:58:43.39 -01:49:10.8 -- not an asteroid (will add it to exclusion list)
06:46:28.56 -04:02:41.2 -- not an asteroid (will add it to exclusion list)
07:02:14.16 +01:01:53.4 -- not an asteroid (will add it to exclusion list)
07:06:05.17 -02:24:58.8 -- not an asteroid (will add it to exclusion list)
07:03:36.19 -03:22:58.6 -- not an asteroid (will add it to exclusion list)
06:52:38.64 -04:12:06.4 -- not an asteroid (will add it to exclusion list)
06:53:52.25 -02:12:22.6 -- not an asteroid (will add it to exclusion list)
06:54:05.49 -01:51:47.4 -- not an asteroid (will add it to exclusion list)
06:59:51.28 -05:11:53.9 -- not an asteroid (will add it to exclusion list)
07:04:05.71 +00:58:06.3 -- not an asteroid (will add it to exclusion list)
06:52:37.15 +00:04:33.8 -- not an asteroid (will add it to exclusion list)
07:01:30.96 -00:10:45.7 -- not an asteroid (will add it to exclusion list)
06:55:40.74 -00:18:33.6 -- not an asteroid (will add it to exclusion list)
07:02:32.47 -00:13:09.9 -- not an asteroid (will add it to exclusion list)
06:46:31.34 +01:08:38.7 -- not an asteroid (will add it to exclusion list)
06:45:14.20 -05:17:04.5 -- not an asteroid (will add it to exclusion list)
06:59:55.77 -04:44:52.9 -- not an asteroid (will add it to exclusion list)
06:58:39.28 -01:55:23.7 -- not an asteroid (will add it to exclusion list)
07:09:13.77 -05:35:54.4 -- not an asteroid (will add it to exclusion list)
07:05:46.02 +01:40:01.9 -- not an asteroid (will add it to exclusion list)
06:57:47.56 +01:28:14.8 -- not an asteroid (will add it to exclusion list)
06:52:01.09 +01:29:17.6 -- not an asteroid (will add it to exclusion list)
06:47:38.70 -04:05:19.3 -- not an asteroid (will add it to exclusion list)
07:09:31.23 -03:28:28.4 -- not an asteroid (will add it to exclusion list)
07:02:23.80 -01:34:40.9 -- not an asteroid (will add it to exclusion list)
06:53:04.60 -05:33:22.4 -- not an asteroid (will add it to exclusion list)
06:59:42.37 -02:10:52.6 -- not an asteroid (will add it to exclusion list)
06:58:08.98 -01:15:49.1 -- not an asteroid (will add it to exclusion list)
07:09:21.66 +01:07:25.9 -- not an asteroid (will add it to exclusion list)
07:01:15.32 -06:13:19.2 -- not an asteroid (will add it to exclusion list)
06:57:44.29 -02:24:17.8 -- not an asteroid (will add it to exclusion list)
07:05:20.07 -02:51:44.0 -- not an asteroid (will add it to exclusion list)
07:04:08.37 +01:01:41.5 -- not an asteroid (will add it to exclusion list)
07:03:33.58 -05:00:26.0 -- not an asteroid (will add it to exclusion list)
06:48:07.73 -00:40:38.5 -- not an asteroid (will add it to exclusion list)
07:09:41.24 -04:22:45.0 -- not an asteroid (will add it to exclusion list)
07:05:04.14 -03:53:19.4 -- not an asteroid (will add it to exclusion list)
06:56:56.53 -01:54:46.4 -- not an asteroid (will add it to exclusion list)
07:07:09.42 -01:15:16.5 -- not an asteroid (will add it to exclusion list)
07:09:10.76 -05:50:44.5 -- not an asteroid (will add it to exclusion list)
07:08:48.66 -03:42:58.5 -- not an asteroid (will add it to exclusion list)
06:49:52.64 -02:41:00.1 -- not an asteroid (will add it to exclusion list)
07:07:57.09 -00:27:58.3 -- not an asteroid (will add it to exclusion list)
07:09:08.56 -01:41:28.2 -- not an asteroid (will add it to exclusion list)
06:48:31.66 -04:05:32.3 -- not an asteroid (will add it to exclusion list)
06:46:14.00 +00:50:44.4 -- not an asteroid (will add it to exclusion list)
06:49:52.45 -02:39:52.4 -- not an asteroid (will add it to exclusion list)
06:58:59.35 -04:37:56.1 -- not an asteroid (will add it to exclusion list)
07:04:10.27 -05:04:54.6 -- not an asteroid (will add it to exclusion list)
06:35:07.45 -03:03:03.8 -- not an asteroid (will add it to exclusion list)
07:02:17.23 -03:49:24.0 -- not an asteroid (will add it to exclusion list)
06:49:22.99 +01:06:39.9 -- not an asteroid (will add it to exclusion list)
06:49:46.88 -00:33:12.0 -- not an asteroid (will add it to exclusion list)
06:58:57.13 -03:00:40.6 -- not an asteroid (will add it to exclusion list)
06:42:58.68 +02:07:38.8 -- not an asteroid (will add it to exclusion list)
06:41:45.21 -01:18:56.8 -- not an asteroid (will add it to exclusion list)
07:05:51.00 -02:05:12.1 -- not an asteroid (will add it to exclusion list)
06:59:00.75 -01:39:59.9 -- not an asteroid (will add it to exclusion list)
06:57:47.67 -01:31:05.7 -- not an asteroid (will add it to exclusion list)
07:07:48.17 +00:24:44.0 -- not an asteroid (will add it to exclusion list)
06:59:36.62 +00:07:20.8 -- not an asteroid (will add it to exclusion list)
06:51:33.07 +00:27:12.9 -- not an asteroid (will add it to exclusion list)
06:51:43.99 +00:27:50.8 -- not an asteroid (will add it to exclusion list)
06:45:12.38 -00:01:52.0 -- not an asteroid (will add it to exclusion list)
06:50:14.56 -00:47:11.7 -- not an asteroid (will add it to exclusion list)
07:06:17.18 +02:00:15.7 -- not an asteroid (will add it to exclusion list)
06:51:05.02 -01:41:33.3 -- not an asteroid (will add it to exclusion list)
07:00:51.52 -03:52:02.8 -- not an asteroid (will add it to exclusion list)
07:06:30.20 -06:00:00.2 -- not an asteroid (will add it to exclusion list)
07:01:48.98 +01:06:04.3 -- not an asteroid (will add it to exclusion list)
06:44:39.70 +00:10:07.3 -- not an asteroid (will add it to exclusion list)
06:56:22.11 -00:53:11.0 -- not an asteroid (will add it to exclusion list)
06:43:08.74 -02:33:59.4 -- not an asteroid (will add it to exclusion list)
06:48:48.76 +00:23:22.6 -- not an asteroid (will add it to exclusion list)
06:42:33.25 -03:28:04.7 -- not an asteroid (will add it to exclusion list)
06:54:43.83 -02:41:21.8 -- not an asteroid (will add it to exclusion list)
06:57:07.90 +00:36:03.3 -- not an asteroid (will add it to exclusion list)
06:49:07.41 -01:40:17.5 -- not an asteroid (will add it to exclusion list)
06:59:43.81 +00:17:13.3 -- not an asteroid (will add it to exclusion list)
06:49:56.12 -02:40:53.6 -- not an asteroid (will add it to exclusion list)
06:42:42.28 -01:42:35.9 -- not an asteroid (will add it to exclusion list)
06:43:36.97 -04:25:01.2 -- not an asteroid (will add it to exclusion list)
06:51:34.34 -01:39:23.3 -- not an asteroid (will add it to exclusion list)
06:55:24.49 -05:54:31.1 -- not an asteroid (will add it to exclusion list)
06:46:12.68 -05:08:48.1 -- not an asteroid (will add it to exclusion list)
06:43:44.34 -05:07:45.9 -- not an asteroid (will add it to exclusion list)
06:50:59.53 +00:13:39.6 -- not an asteroid (will add it to exclusion list)
07:01:28.13 -05:15:07.2 -- not an asteroid (will add it to exclusion list)
07:01:22.85 -05:01:11.0 -- not an asteroid (will add it to exclusion list)
06:41:27.04 -01:19:01.9 -- not an asteroid (will add it to exclusion list)
07:08:59.19 -00:34:32.2 -- not an asteroid (will add it to exclusion list)
06:45:33.74 -00:26:16.5 -- not an asteroid (will add it to exclusion list)
06:41:21.26 -01:43:18.6 -- not an asteroid (will add it to exclusion list)
06:57:35.85 +01:13:54.0 -- not an asteroid (will add it to exclusion list)
06:50:41.51 -00:31:43.8 -- not an asteroid (will add it to exclusion list)
06:49:56.12 -02:17:03.1 -- not an asteroid (will add it to exclusion list)
06:54:17.85 -04:54:46.6 -- not an asteroid (will add it to exclusion list)
06:48:57.08 -03:30:57.5 -- not an asteroid (will add it to exclusion list)
06:43:55.57 -05:04:00.5 -- not an asteroid (will add it to exclusion list)
07:01:15.48 -00:32:58.4 -- not an asteroid (will add it to exclusion list)
06:38:41.64 +01:56:39.6 -- not an asteroid (will add it to exclusion list)
07:05:35.96 -05:43:55.9 -- not an asteroid (will add it to exclusion list)
06:47:15.17 -05:48:24.0 -- not an asteroid (will add it to exclusion list)
06:48:34.70 -03:13:29.3 -- not an asteroid (will add it to exclusion list)
06:57:27.90 -05:05:42.5 -- not an asteroid (will add it to exclusion list)
06:45:17.66 +00:43:38.6 -- not an asteroid (will add it to exclusion list)
07:05:00.39 -01:12:33.6 -- not an asteroid (will add it to exclusion list)
06:51:28.50 -00:06:28.4 -- not an asteroid (will add it to exclusion list)
07:03:46.90 -01:04:50.9 -- not an asteroid (will add it to exclusion list)
06:48:23.31 -05:30:24.5 -- not an asteroid (will add it to exclusion list)
06:53:13.94 -04:35:48.9 -- not an asteroid (will add it to exclusion list)
06:47:44.87 +00:19:24.7 -- not an asteroid (will add it to exclusion list)
06:49:24.69 -00:56:16.7 -- not an asteroid (will add it to exclusion list)
06:58:20.47 -00:32:37.7 -- not an asteroid (will add it to exclusion list)
06:56:35.74 +00:19:16.8 -- not an asteroid (will add it to exclusion list)
07:00:15.99 +01:37:06.2 -- not an asteroid (will add it to exclusion list)
06:55:15.98 +00:20:60.0 -- not an asteroid (will add it to exclusion list)
07:07:24.04 -01:20:23.1 -- not an asteroid (will add it to exclusion list)
07:01:19.02 +01:03:48.3 -- not an asteroid (will add it to exclusion list)
06:52:28.75 -04:22:31.2 -- not an asteroid (will add it to exclusion list)
06:52:34.77 +00:32:34.7 -- not an asteroid (will add it to exclusion list)
06:50:01.96 +00:45:50.3 -- not an asteroid (will add it to exclusion list)
06:56:58.64 +00:23:51.1 -- not an asteroid (will add it to exclusion list)
06:57:11.64 -01:07:43.9 -- not an asteroid (will add it to exclusion list)
07:04:51.63 -02:12:04.3 -- not an asteroid (will add it to exclusion list)
06:47:46.59 -02:22:19.2 -- not an asteroid (will add it to exclusion list)
06:41:55.53 -00:07:52.6 -- not an asteroid (will add it to exclusion list)
06:38:28.93 -06:01:35.0 -- not an asteroid (will add it to exclusion list)
06:44:20.03 +01:40:51.7 -- not an asteroid (will add it to exclusion list)
06:53:47.32 -02:38:43.9 -- not an asteroid (will add it to exclusion list)
07:07:30.06 -05:41:17.4 -- not an asteroid (will add it to exclusion list)
06:47:59.64 -01:20:54.3 -- not an asteroid (will add it to exclusion list)
06:39:41.58 +00:27:18.9 -- not an asteroid (will add it to exclusion list)
06:50:45.39 -02:12:09.1 -- not an asteroid (will add it to exclusion list)
07:02:14.25 -00:34:58.5 -- not an asteroid (will add it to exclusion list)
07:00:01.85 -04:09:56.7 -- not an asteroid (will add it to exclusion list)
06:52:59.53 -03:53:49.7 -- not an asteroid (will add it to exclusion list)
06:58:34.20 -01:38:07.0 -- not an asteroid (will add it to exclusion list)
07:07:29.55 +01:15:33.2 -- not an asteroid (will add it to exclusion list)
06:55:00.90 -01:15:39.7 -- not an asteroid (will add it to exclusion list)
06:52:56.39 -02:22:52.9 -- not an asteroid (will add it to exclusion list)
06:38:39.62 +01:56:42.4 -- not an asteroid (will add it to exclusion list)
06:59:11.07 -01:18:50.5 -- not an asteroid (will add it to exclusion list)
06:53:59.16 -01:54:56.0 -- not an asteroid (will add it to exclusion list)
06:37:40.99 -03:18:48.9 -- not an asteroid (will add it to exclusion list)
07:00:30.86 -02:55:26.7 -- not an asteroid (will add it to exclusion list)
06:58:34.80 -01:38:24.4 -- not an asteroid (will add it to exclusion list)
07:02:16.89 -05:05:04.7 -- not an asteroid (will add it to exclusion list)
07:08:50.18 -03:10:51.0 -- not an asteroid (will add it to exclusion list)
06:49:52.53 +01:17:48.6 -- not an asteroid (will add it to exclusion list)
07:00:20.22 +01:48:28.5 -- not an asteroid (will add it to exclusion list)
07:05:23.70 -01:58:45.1 -- not an asteroid (will add it to exclusion list)
06:45:19.63 +01:14:09.9 -- not an asteroid (will add it to exclusion list)
07:02:16.17 -02:43:01.8 -- not an asteroid (will add it to exclusion list)
06:55:28.08 -04:33:51.7 -- not an asteroid (will add it to exclusion list)
06:56:38.66 -01:07:55.9 -- not an asteroid (will add it to exclusion list)
07:04:55.72 -05:17:03.6 -- not an asteroid (will add it to exclusion list)
07:02:58.20 -02:30:17.1 -- not an asteroid (will add it to exclusion list)
06:45:26.17 -00:11:49.7 -- not an asteroid (will add it to exclusion list)
07:02:25.77 -04:08:33.5 -- not an asteroid (will add it to exclusion list)
06:58:30.33 -01:38:04.9 -- not an asteroid (will add it to exclusion list)
06:58:09.49 -01:01:48.7 -- not an asteroid (will add it to exclusion list)
06:47:15.19 +00:57:18.3 -- not an asteroid (will add it to exclusion list)
07:03:41.18 -04:17:19.7 -- not an asteroid (will add it to exclusion list)
06:54:43.78 -02:51:58.3 -- not an asteroid (will add it to exclusion list)
06:40:44.67 -01:31:43.2 -- not an asteroid (will add it to exclusion list)
06:59:41.69 +01:51:43.3 -- not an asteroid (will add it to exclusion list)
06:57:56.90 -01:46:47.0 -- not an asteroid (will add it to exclusion list)
06:36:38.18 -00:15:15.0 -- not an asteroid (will add it to exclusion list)
06:58:19.61 -01:55:23.3 -- not an asteroid (will add it to exclusion list)
07:06:38.71 +01:16:42.5 -- not an asteroid (will add it to exclusion list)
07:07:45.52 -00:30:37.7 -- not an asteroid (will add it to exclusion list)
06:52:06.83 -04:04:30.1 -- not an asteroid (will add it to exclusion list)
06:48:03.89 +01:52:53.7 -- not an asteroid (will add it to exclusion list)
06:43:53.86 +01:01:55.1 -- not an asteroid (will add it to exclusion list)
07:02:45.55 -04:03:43.9 -- not an asteroid (will add it to exclusion list)
06:53:09.57 -01:41:52.7 -- not an asteroid (will add it to exclusion list)
06:55:30.26 -05:25:59.0 -- not an asteroid (will add it to exclusion list)
06:54:15.66 -05:56:34.7 -- not an asteroid (will add it to exclusion list)
07:09:08.15 -00:17:49.6 -- not an asteroid (will add it to exclusion list)
06:53:19.90 -02:43:44.0 -- not an asteroid (will add it to exclusion list)
06:53:47.66 -05:01:30.8 -- not an asteroid (will add it to exclusion list)
07:03:04.29 -03:35:09.1 -- not an asteroid (will add it to exclusion list)
07:06:17.21 -01:42:55.2 -- not an asteroid (will add it to exclusion list)
06:57:35.00 -00:39:10.9 -- not an asteroid (will add it to exclusion list)
07:06:11.24 -01:44:21.0 -- not an asteroid (will add it to exclusion list)
06:54:20.75 +00:46:57.4 -- not an asteroid (will add it to exclusion list)
06:54:38.30 +00:38:49.8 -- not an asteroid (will add it to exclusion list)
06:55:22.13 -00:31:19.0 -- not an asteroid (will add it to exclusion list)
07:07:15.26 -02:45:45.9 -- not an asteroid (will add it to exclusion list)
06:55:22.82 -02:54:14.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.45 -03:03:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:38.18 -00:15:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:40.99 -03:18:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:28.93 -06:01:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:39.62 +01:56:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:41.64 +01:56:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:39:41.58 +00:27:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:44.67 -01:31:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.26 -01:43:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.04 -01:19:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:45.21 -01:18:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:55.53 -00:07:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.25 -03:28:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:37.07 +00:51:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:42.28 -01:42:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:58.68 +02:07:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:08.74 -02:33:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:14.44 +01:58:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:28.37 -00:41:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:35.56 +02:06:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:36.97 -04:25:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:44.34 -05:07:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:46.58 -05:42:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:53.86 +01:01:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:55.57 -05:04:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:20.03 +01:40:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.70 +00:10:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:49.26 +00:56:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:56.02 -05:29:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:11.99 +00:14:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.38 -00:01:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:13.10 -00:39:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:14.20 -05:17:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.66 +00:43:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:19.63 +01:14:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:26.17 -00:11:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:33.74 -00:26:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:12.68 -05:08:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:14.00 +00:50:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:28.56 -04:02:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.34 +01:08:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:32.65 -01:51:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:15.17 -05:48:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:15.19 +00:57:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:38.70 -04:05:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:44.87 +00:19:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:46.59 -02:22:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:59.64 -01:20:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:03.89 +01:52:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:07.73 -00:40:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:10.30 -01:11:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:23.31 -05:30:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:31.66 -04:05:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:34.70 -03:13:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:48.76 +00:23:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:57.08 -03:30:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.41 -01:40:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:22.99 +01:06:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:24.69 -00:56:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:46.88 -00:33:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.45 -02:39:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.53 +01:17:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.64 -02:41:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.12 -02:17:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.12 -02:40:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:01.96 +00:45:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:08.87 -05:03:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:14.56 -00:47:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:18.59 -02:39:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:27.41 -02:58:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.51 -00:31:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:45.39 -02:12:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:57.46 -01:59:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.53 +00:13:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:05.02 -01:41:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.50 -00:06:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:33.07 +00:27:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.34 -01:39:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:43.99 +00:27:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:01.09 +01:29:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:06.83 -04:04:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:28.75 -04:22:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:34.77 +00:32:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:37.15 +00:04:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:38.64 -04:12:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:48.53 +00:32:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:56.39 -02:22:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:59.53 -03:53:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.60 -05:33:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:09.57 -01:41:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:13.94 -04:35:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:19.90 -02:43:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:34.00 -04:54:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.32 -02:38:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.66 -05:01:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:52.25 -02:12:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:59.16 -01:54:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:05.49 -01:51:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:15.66 -05:56:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:17.53 -00:33:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:17.85 -04:54:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:20.75 +00:46:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:25.07 -05:50:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:38.30 +00:38:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:43.78 -02:51:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:43.83 -02:41:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:00.90 -01:15:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:15.98 +00:20:60.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:22.13 -00:31:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:22.82 -02:54:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:24.49 -05:54:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:28.08 -04:33:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:30.26 -05:25:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:40.74 -00:18:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.11 -00:53:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:35.74 +00:19:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:38.66 -01:07:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:56.53 -01:54:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:58.64 +00:23:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:07.03 -02:14:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:07.90 +00:36:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.64 -01:07:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:27.90 -05:05:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.00 -00:39:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.85 +01:13:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:44.29 -02:24:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.56 +01:28:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:47.67 -01:31:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:48.02 -02:04:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:56.90 -01:46:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:08.98 -01:15:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:09.49 -01:01:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:19.61 -01:55:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:20.47 -00:32:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:30.33 -01:38:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.20 -01:38:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.80 -01:38:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.28 -01:55:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:42.27 -06:03:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:43.39 -01:49:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.13 -03:00:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:59.35 -04:37:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.75 -01:39:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:05.20 -00:46:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:11.07 -01:18:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:33.19 -02:59:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:36.62 +00:07:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:41.69 +01:51:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:42.37 -02:10:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:43.81 +00:17:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:50.28 -01:50:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:51.28 -05:11:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:55.77 -04:44:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:01.85 -04:09:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:15.99 +01:37:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:20.22 +01:48:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:30.86 -02:55:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:42.70 -01:17:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:43.17 -00:59:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:51.52 -03:52:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:08.52 -05:31:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.32 -06:13:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.48 -00:32:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:16.54 -02:28:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:19.02 +01:03:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:22.85 -05:01:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:28.13 -05:15:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:30.96 -00:10:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:48.98 +01:06:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.16 +01:01:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:14.25 -00:34:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:16.17 -02:43:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:16.89 -05:05:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:17.23 -03:49:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.80 -01:34:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:25.77 -04:08:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:32.47 -00:13:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:45.55 -04:03:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:58.20 -02:30:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.29 -03:35:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:33.58 -05:00:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.19 -03:22:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:37.03 -00:12:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:41.18 -04:17:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:46.90 -01:04:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:05.71 +00:58:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:08.37 +01:01:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:10.27 -05:04:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:23.82 -02:15:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.63 -02:12:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:55.72 -05:17:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:00.39 -01:12:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:04.14 -03:53:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:16.10 -05:50:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:20.07 -02:51:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:23.70 -01:58:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:29.09 -02:26:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:35.96 -05:43:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:46.02 +01:40:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:51.00 -02:05:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:05.17 -02:24:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:11.24 -01:44:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:17.18 +02:00:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:17.21 -01:42:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:30.20 -06:00:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:38.71 +01:16:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:42.72 -04:01:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:09.42 -01:15:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.26 -02:45:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:24.04 -01:20:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:29.55 +01:15:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:30.06 -05:41:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:34.54 -03:27:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:45.52 -00:30:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:48.17 +00:24:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:57.09 -00:27:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:16.87 -00:08:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.66 -03:42:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:50.18 -03:10:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:59.19 -00:34:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:08.15 -00:17:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:08.56 -01:41:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.76 -05:50:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:13.77 -05:35:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:21.66 +01:07:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:24.60 -02:17:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:31.23 -03:28:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:41.24 -04:22:45.0 -- 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)
06:35:07.45 -03:03:03.8 -- not a known variable star
06:36:38.18 -00:15:15.0 -- not a known variable star
06:37:40.99 -03:18:48.9 -- not a known variable star
06:38:28.93 -06:01:35.0 -- not a known variable star
06:38:39.62 +01:56:42.4 -- not a known variable star
06:38:41.64 +01:56:39.6 -- not a known variable star
06:39:41.58 +00:27:18.9 -- not a known variable star
06:40:44.67 -01:31:43.2 -- not a known variable star
06:41:21.26 -01:43:18.6 -- not a known variable star
06:41:27.04 -01:19:01.9 -- a known variable star
06:41:45.21 -01:18:56.8 -- a known variable star
06:41:55.53 -00:07:52.6 -- a known variable star
06:42:33.25 -03:28:04.7 -- not a known variable star
06:42:37.07 +00:51:08.7 -- not a known variable star
06:42:42.28 -01:42:35.9 -- not a known variable star
06:42:58.68 +02:07:38.8 -- a known variable star
06:43:08.74 -02:33:59.4 -- not a known variable star
06:43:14.44 +01:58:18.5 -- not a known variable star
06:43:28.37 -00:41:03.8 -- a known variable star
06:43:35.56 +02:06:58.4 -- not a known variable star
06:43:36.97 -04:25:01.2 -- a known variable star
06:43:44.34 -05:07:45.9 -- a known variable star
06:43:46.58 -05:42:06.3 -- not a known variable star
06:43:53.86 +01:01:55.1 -- a known variable star
06:43:55.57 -05:04:00.5 -- not a known variable star
06:44:20.03 +01:40:51.7 -- not a known variable star
06:44:39.70 +00:10:07.3 -- a known variable star
06:44:49.26 +00:56:55.9 -- not a known variable star
06:44:56.02 -05:29:00.7 -- a known variable star
06:45:11.99 +00:14:17.9 -- not a known variable star
06:45:12.38 -00:01:52.0 -- not a known variable star
06:45:13.10 -00:39:25.7 -- not a known variable star
06:45:14.20 -05:17:04.5 -- a known variable star
06:45:17.66 +00:43:38.6 -- not a known variable star
06:45:19.63 +01:14:09.9 -- not a known variable star
06:45:26.17 -00:11:49.7 -- not a known variable star
06:45:33.74 -00:26:16.5 -- a known variable star
06:46:12.68 -05:08:48.1 -- not a known variable star
06:46:14.00 +00:50:44.4 -- not a known variable star
06:46:28.56 -04:02:41.2 -- not a known variable star
06:46:31.34 +01:08:38.7 -- not a known variable star
06:46:32.65 -01:51:12.9 -- not a known variable star
06:47:15.17 -05:48:24.0 -- not a known variable star
06:47:15.19 +00:57:18.3 -- not a known variable star
06:47:38.70 -04:05:19.3 -- not a known variable star
06:47:44.87 +00:19:24.7 -- not a known variable star
06:47:46.59 -02:22:19.2 -- not a known variable star
06:47:59.64 -01:20:54.3 -- not a known variable star
06:48:03.89 +01:52:53.7 -- not a known variable star
06:48:07.73 -00:40:38.5 -- not a known variable star
06:48:10.30 -01:11:30.7 -- a known variable star
06:48:23.31 -05:30:24.5 -- not a known variable star
06:48:31.66 -04:05:32.3 -- a known variable star
06:48:34.70 -03:13:29.3 -- not a known variable star
06:48:48.76 +00:23:22.6 -- a known variable star
06:48:57.08 -03:30:57.5 -- not a known variable star
06:49:07.41 -01:40:17.5 -- not a known variable star
06:49:22.99 +01:06:39.9 -- a known variable star
06:49:24.69 -00:56:16.7 -- not a known variable star
06:49:46.88 -00:33:12.0 -- not a known variable star
06:49:52.45 -02:39:52.4 -- not a known variable star
06:49:52.53 +01:17:48.6 -- not a known variable star
06:49:52.64 -02:41:00.1 -- not a known variable star
06:49:56.12 -02:17:03.1 -- not a known variable star
06:49:56.12 -02:40:53.6 -- not a known variable star
06:50:01.96 +00:45:50.3 -- not a known variable star
06:50:08.87 -05:03:54.2 -- a known variable star
06:50:14.56 -00:47:11.7 -- not a known variable star
06:50:18.59 -02:39:12.6 -- not a known variable star
06:50:27.41 -02:58:41.8 -- not a known variable star
06:50:41.51 -00:31:43.8 -- not a known variable star
06:50:45.39 -02:12:09.1 -- not a known variable star
06:50:57.46 -01:59:56.3 -- not a known variable star
06:50:59.53 +00:13:39.6 -- not a known variable star
06:51:05.02 -01:41:33.3 -- a known variable star
06:51:28.50 -00:06:28.4 -- not a known variable star
06:51:33.07 +00:27:12.9 -- a known variable star
06:51:34.34 -01:39:23.3 -- not a known variable star
06:51:43.99 +00:27:50.8 -- not a known variable star
06:52:01.09 +01:29:17.6 -- not a known variable star
06:52:06.83 -04:04:30.1 -- a known variable star
06:52:28.75 -04:22:31.2 -- not a known variable star
06:52:34.77 +00:32:34.7 -- not a known variable star
06:52:37.15 +00:04:33.8 -- not a known variable star
06:52:38.64 -04:12:06.4 -- not a known variable star
06:52:48.53 +00:32:44.3 -- not a known variable star
06:52:56.39 -02:22:52.9 -- not a known variable star
06:52:59.53 -03:53:49.7 -- not a known variable star
06:53:04.60 -05:33:22.4 -- not a known variable star
06:53:09.57 -01:41:52.7 -- not a known variable star
06:53:13.94 -04:35:48.9 -- not a known variable star
06:53:19.90 -02:43:44.0 -- not a known variable star
06:53:34.00 -04:54:50.0 -- a known variable star
06:53:47.32 -02:38:43.9 -- not a known variable star
06:53:47.66 -05:01:30.8 -- not a known variable star
06:53:52.25 -02:12:22.6 -- not a known variable star
06:53:59.16 -01:54:56.0 -- not a known variable star
06:54:05.49 -01:51:47.4 -- not a known variable star
06:54:15.66 -05:56:34.7 -- a known variable star
06:54:17.53 -00:33:49.3 -- a known variable star
06:54:17.85 -04:54:46.6 -- not a known variable star
06:54:20.75 +00:46:57.4 -- a known variable star
06:54:25.07 -05:50:48.5 -- not a known variable star
06:54:38.30 +00:38:49.8 -- not a known variable star
06:54:43.78 -02:51:58.3 -- not a known variable star
06:54:43.83 -02:41:21.8 -- not a known variable star
06:55:00.90 -01:15:39.7 -- a known variable star
06:55:15.98 +00:20:60.0 -- not a known variable star
06:55:22.13 -00:31:19.0 -- not a known variable star
06:55:22.82 -02:54:14.1 -- not a known variable star
06:55:24.49 -05:54:31.1 -- not a known variable star
06:55:28.08 -04:33:51.7 -- not a known variable star
06:55:30.26 -05:25:59.0 -- not a known variable star
06:55:40.74 -00:18:33.6 -- not a known variable star
06:56:22.11 -00:53:11.0 -- a known variable star
06:56:35.74 +00:19:16.8 -- not a known variable star
06:56:38.66 -01:07:55.9 -- not a known variable star
06:56:56.53 -01:54:46.4 -- a known variable star
06:56:58.64 +00:23:51.1 -- not a known variable star
06:57:07.03 -02:14:45.0 -- not a known variable star
06:57:07.90 +00:36:03.3 -- not a known variable star
06:57:11.64 -01:07:43.9 -- a known variable star
06:57:27.90 -05:05:42.5 -- not a known variable star
06:57:35.00 -00:39:10.9 -- not a known variable star
06:57:35.85 +01:13:54.0 -- a known variable star
06:57:44.29 -02:24:17.8 -- not a known variable star
06:57:47.56 +01:28:14.8 -- not a known variable star
06:57:47.67 -01:31:05.7 -- a known variable star
06:57:48.02 -02:04:24.0 -- not a known variable star
06:57:56.90 -01:46:47.0 -- a known variable star
06:58:08.98 -01:15:49.1 -- not a known variable star
06:58:09.49 -01:01:48.7 -- not a known variable star
06:58:19.61 -01:55:23.3 -- not a known variable star
06:58:20.47 -00:32:37.7 -- not a known variable star
06:58:30.33 -01:38:04.9 -- not a known variable star
06:58:34.20 -01:38:07.0 -- not a known variable star
06:58:34.80 -01:38:24.4 -- not a known variable star
06:58:39.28 -01:55:23.7 -- not a known variable star
06:58:42.27 -06:03:35.1 -- not a known variable star
06:58:43.39 -01:49:10.8 -- not a known variable star
06:58:57.13 -03:00:40.6 -- not a known variable star
06:58:59.35 -04:37:56.1 -- not a known variable star
06:59:00.75 -01:39:59.9 -- not a known variable star
06:59:05.20 -00:46:04.2 -- not a known variable star
06:59:11.07 -01:18:50.5 -- not a known variable star
06:59:33.19 -02:59:48.1 -- not a known variable star
06:59:36.62 +00:07:20.8 -- not a known variable star
06:59:41.69 +01:51:43.3 -- not a known variable star
06:59:42.37 -02:10:52.6 -- a known variable star
06:59:43.81 +00:17:13.3 -- a known variable star
06:59:50.28 -01:50:12.9 -- not a known variable star
06:59:51.28 -05:11:53.9 -- a known variable star
06:59:55.77 -04:44:52.9 -- not a known variable star
07:00:01.85 -04:09:56.7 -- not a known variable star
07:00:15.99 +01:37:06.2 -- not a known variable star
07:00:20.22 +01:48:28.5 -- not a known variable star
07:00:30.86 -02:55:26.7 -- not a known variable star
07:00:42.70 -01:17:01.4 -- a known variable star
07:00:43.17 -00:59:23.0 -- not a known variable star
07:00:51.52 -03:52:02.8 -- not a known variable star
07:01:08.52 -05:31:36.8 -- a known variable star
07:01:15.32 -06:13:19.2 -- not a known variable star
07:01:15.48 -00:32:58.4 -- a known variable star
07:01:16.54 -02:28:43.2 -- not a known variable star
07:01:19.02 +01:03:48.3 -- not a known variable star
07:01:22.85 -05:01:11.0 -- not a known variable star
07:01:28.13 -05:15:07.2 -- a known variable star
07:01:30.96 -00:10:45.7 -- not a known variable star
07:01:48.98 +01:06:04.3 -- not a known variable star
07:02:14.16 +01:01:53.4 -- a known variable star
07:02:14.25 -00:34:58.5 -- not a known variable star
07:02:16.17 -02:43:01.8 -- not a known variable star
07:02:16.89 -05:05:04.7 -- not a known variable star
07:02:17.23 -03:49:24.0 -- not a known variable star
07:02:23.80 -01:34:40.9 -- not a known variable star
07:02:25.77 -04:08:33.5 -- not a known variable star
07:02:32.47 -00:13:09.9 -- not a known variable star
07:02:45.55 -04:03:43.9 -- not a known variable star
07:02:58.20 -02:30:17.1 -- not a known variable star
07:03:04.29 -03:35:09.1 -- not a known variable star
07:03:33.58 -05:00:26.0 -- not a known variable star
07:03:36.19 -03:22:58.6 -- not a known variable star
07:03:37.03 -00:12:38.1 -- not a known variable star
07:03:41.18 -04:17:19.7 -- a known variable star
07:03:46.90 -01:04:50.9 -- not a known variable star
07:04:05.71 +00:58:06.3 -- not a known variable star
07:04:08.37 +01:01:41.5 -- not a known variable star
07:04:10.27 -05:04:54.6 -- not a known variable star
07:04:23.82 -02:15:16.5 -- a known variable star
07:04:51.63 -02:12:04.3 -- not a known variable star
07:04:55.72 -05:17:03.6 -- not a known variable star
07:05:00.39 -01:12:33.6 -- a known variable star
07:05:04.14 -03:53:19.4 -- not a known variable star
07:05:16.10 -05:50:54.2 -- not a known variable star
07:05:20.07 -02:51:44.0 -- a known variable star
07:05:23.70 -01:58:45.1 -- a known variable star
07:05:29.09 -02:26:14.4 -- a known variable star
07:05:35.96 -05:43:55.9 -- not a known variable star
07:05:46.02 +01:40:01.9 -- a known variable star
07:05:51.00 -02:05:12.1 -- not a known variable star
07:06:05.17 -02:24:58.8 -- not a known variable star
07:06:11.24 -01:44:21.0 -- not a known variable star
07:06:17.18 +02:00:15.7 -- not a known variable star
07:06:17.21 -01:42:55.2 -- not a known variable star
07:06:30.20 -06:00:00.2 -- a known variable star
07:06:38.71 +01:16:42.5 -- a known variable star
07:06:42.72 -04:01:01.9 -- a known variable star
07:07:09.42 -01:15:16.5 -- a known variable star
07:07:15.26 -02:45:45.9 -- not a known variable star
07:07:24.04 -01:20:23.1 -- a known variable star
07:07:29.55 +01:15:33.2 -- not a known variable star
07:07:30.06 -05:41:17.4 -- not a known variable star
07:07:34.54 -03:27:34.5 -- not a known variable star
07:07:45.52 -00:30:37.7 -- not a known variable star
07:07:48.17 +00:24:44.0 -- not a known variable star
07:07:57.09 -00:27:58.3 -- not a known variable star
07:08:16.87 -00:08:18.0 -- a known variable star
07:08:48.66 -03:42:58.5 -- not a known variable star
07:08:50.18 -03:10:51.0 -- not a known variable star
07:08:59.19 -00:34:32.2 -- a known variable star
07:09:08.15 -00:17:49.6 -- not a known variable star
07:09:08.56 -01:41:28.2 -- a known variable star
07:09:10.76 -05:50:44.5 -- a known variable star
07:09:13.77 -05:35:54.4 -- a known variable star
07:09:21.66 +01:07:25.9 -- a known variable star
07:09:24.60 -02:17:49.3 -- not a known variable star
07:09:31.23 -03:28:28.4 -- not a known variable star
07:09:41.24 -04:22:45.0 -- not a known variable star
Found 171 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
228 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 228 (excluding asteroids and hot pixels, 171 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)2461146.60977953 -observatory V36
00:07:51.66 -01:59:56.3 Mercury (0.0mag)
03:09:10.81 +17:53:56.6 Venus (-3.9mag)
00:18:09.12 +00:53:56.9 Mars (1.2mag)
07:12:40.84 +22:46:09.2 Jupiter (-2.1mag)
00:29:13.80 +00:49:17.2 Saturn (0.9mag)
03:47:43.20 +19:47:33.1 Uranus (5.8mag)
00:10:51.27 -00:15:16.9 Neptune (7.8mag)
20:33:45.55 -22:52:36.1 Pluto (14.5mag)
00:19:27.62 +04:31:45.1 Moon (-8.6mag)
-rw-r--r-- 1 apache apache 361 Apr 15 23:34 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461146.60977953:
07:12:41.96 +22:46:09.3 Io (5.8mag)
07:12:46.12 +22:46:00.5 Europa (5.9mag)
07:12:57.91 +22:45:29.7 Ganymede (5.4mag)
07:13:16.21 +22:44:56.9 Callisto (6.6mag)
07:16:00.79 +22:33:43.6 Himalia (15.3mag)
07:12:39.31 +22:46:10.3 Thebe (16.2mag)
07:16:12.32 +23:03:55.8 Elara (17.3mag)
07:11:34.17 +23:26:06.1 Pasiphae (17.4mag)
07:21:00.40 +22:44:11.1 Carme (18.5mag)
00:29:14.36 +00:49:43.4 Titan (8.8mag)
00:29:12.24 +00:49:21.5 Rhea (10.1mag)
00:28:53.62 +00:49:25.6 Iapetus (11.5mag)
00:29:21.73 +00:49:37.3 Hyperion (14.8mag)
00:30:50.61 +00:58:04.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 15 23:34 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461146.60977953:
15:38:58.60 -16:18:44.8 JWST
13:12:17.43 +54:04:17.7 Chandra
07:50:56.90 -33:31:51.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 15 23:34 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461146.60977953 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:02.91 -28:47:06.9 13.9mag P/2010 H2 (Vales)
05:06:48.79 -69:39:24.1 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:28.17 +31:26:17.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:25.53 +10:33:38.5 17.6mag C/2021 G2 (ATLAS)
23:10:15.19 +29:13:59.5 17.1mag C/2022 E2 (ATLAS)
04:29:21.82 +26:02:29.4 16.0mag C/2022 N2 (PANSTARRS)
09:03:26.62 +32:01:06.3 16.2mag C/2022 QE78 (ATLAS)
08:31:05.40 -00:08:29.3 17.3mag C/2022 R6 (PANSTARRS)
18:53:42.36 +18:32:29.8 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:38.39 -11:31:11.9 17.5mag P/2023 B1 (PANSTARRS)
09:07:35.08 -11:51:56.0 17.6mag C/2023 F3 (ATLAS)
21:54:19.51 +62:54:45.6 17.5mag C/2023 H5 (Lemmon)
19:19:06.33 -03:44:03.3 14.1mag C/2023 R1 (PANSTARRS)
21:32:19.31 +85:55:35.4 17.8mag C/2023 X2 (Lemmon)
06:17:56.87 +63:30:45.4 17.2mag C/2024 A1 (ATLAS)
05:13:30.70 +18:20:42.5 11.1mag C/2024 E1 (Wierzchos)
16:19:12.40 +06:24:30.4 17.4mag C/2024 G6 (ATLAS)
20:20:50.56 +15:18:14.6 14.6mag C/2024 J3 (ATLAS)
03:26:27.98 -22:22:07.8 16.3mag C/2024 T5 (ATLAS)
05:16:48.30 +45:15:50.0 17.7mag C/2025 J1 (Borisov)
13:38:22.89 +45:33:45.4 15.2mag C/2025 L1 (ATLAS)
03:25:26.83 -26:13:43.9 17.8mag C/2025 Q3 (ATLAS)
23:44:21.90 +18:34:35.5 8.5mag C/2025 R3 (PANSTARRS)
12:54:04.28 +03:01:10.2 17.4mag C/2025 Y1 (ATLAS)
03:28:50.46 +02:36:29.6 13.3mag C/2026 A1 (MAPS)
23:59:53.45 +37:14:23.3 14.6mag C/2026 B2 (Sun-Gao)
18:43:08.90 -09:42:47.3 11.8mag 10P/Tempel
15:00:09.67 +03:11:52.7 14.0mag 24P/Schaumasse
11:02:46.40 -01:31:21.4 15.7mag 29P/Schwassmann-Wachmann
18:00:59.74 -09:36:21.5 17.9mag 40P/Vaisala
10:37:33.63 -04:05:24.3 16.9mag 43P/Wolf-Harrington
01:48:50.55 +17:30:23.1 17.2mag 47P/Ashbrook-Jackson
07:10:57.99 +36:59:22.3 17.0mag 63P/Wild
23:29:11.80 -11:26:15.5 15.7mag 65P/Gunn
04:03:32.44 +21:17:35.1 15.9mag 76P/West-Kohoutek-Ikemura
01:05:48.97 +08:15:01.2 14.3mag 78P/Gehrels
23:03:20.09 -09:21:31.2 14.6mag 88P/Howell
02:10:42.53 +20:40:18.5 15.1mag 93P/Lovas
04:55:00.54 +32:17:37.8 16.2mag 123P/West-Hartley
08:28:29.51 +38:18:38.7 16.2mag 124P/Mrkos
02:33:23.06 +14:22:56.3 16.4mag 128P/Shoemaker-Holt
02:47:45.09 +14:30:24.2 17.5mag 131P/Mueller
01:26:44.33 +13:16:36.5 10.6mag 141P/Machholz
01:35:39.19 +04:54:54.2 10.6mag 141P-A/Machholz
00:20:53.66 +00:49:12.7 12.8mag 141P-D/Machholz
02:05:59.49 +06:40:26.9 17.8mag 141P-I/Machholz
01:02:40.96 -01:28:14.2 15.1mag 162P/SidingSpring
14:51:14.43 -00:03:23.5 17.6mag 210P/Christensen
21:39:09.81 -11:25:19.4 17.6mag 218P/LINEAR
17:16:35.80 -13:55:11.8 16.1mag 235P/LINEAR
05:34:43.12 +34:42:27.0 16.8mag 240P/NEAT
07:38:32.84 -05:09:18.8 17.7mag 242P/Spahr
22:17:10.88 -20:57:03.2 17.9mag 260P/McNaught
01:58:24.71 +20:29:18.3 18.0mag 295P/LINEAR
15:42:36.27 +06:59:52.1 17.5mag 391P/Kowalski
07:34:14.26 +21:21:59.2 17.7mag 450P/LONEOS
05:36:01.81 +45:01:35.1 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 15 23:34 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
15:25:54.99 +07:49:24.50 2026-04-12.14 16.96
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
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
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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 15 23:34 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:52:32.558 +54:28:28.21 AT 2026iyo 2026-04-07.50 19.8736
12:10:51.131 -15:24:05.80 AT 2026iyn 2026-04-07.49 19.8
10:03:32.464 +00:47:38.92 AT 2026iym 2026-04-09.07 21.7842
09:57:46.577 +02:32:54.17 AT 2026iyl 2026-04-09.07 21.1159
12:09:21.288 -14:20:40.69 AT 2026iyk 2026-02-24.42 19.0617
11:32:15.323 +26:34:23.97 AT 2026iyi 2026-04-07.27 20.0038
08:41:36.643 +41:14:51.53 AT 2026iyh 2026-03-18.28 20.5874
11:10:47.748 -02:27:00.61 AT 2026iyg 2026-04-07.26 20.12
11:41:25.329 -11:32:16.55 AT 2026iyf 2026-04-07.25 20.8489
09:58:35.594 -17:44:37.57 AT 2026iye 2026-04-08.19 19.4848
07:48:08.582 +43:35:35.35 AT 2026iyd 2026-04-05.16 19.8382
11:13:43.729 +21:50:31.84 AT 2026iyc 2026-04-05.18 20.0005
08:02:45.458 +40:40:22.73 AT 2026iyb 2026-03-26.18 20.4831
13:05:52.496 +64:22:32.75 AT 2026iya 2026-03-08.94 19.29
05:15:26.423 -02:54:24.54 AT 2026ixz 2026-04-08.14 19.1905
14:04:24.118 +43:40:15.80 AT 2026ixt 2026-04-08.93 19.74
13:12:41.279 +38:05:24.08 AT 2026ixs 2026-04-08.93 20.18
13:21:56.843 -04:01:33.33 AT 2026ixr 2026-04-08.90 19.48
12:04:52.343 +69:44:57.80 AT 2026ixq 2026-04-08.89 19.03
21:31:46.671 +04:33:36.35 AT 2026ixp 2026-04-08.51 19.1697
-rw-r--r-- 1 apache apache 30K Apr 15 23:34 tns_transients_list.txt
