This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.7588+42.7450,2461135.6545,13.69,0.05,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
ATO J089.7588+42.7450 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J060018.79+475603.4,2461135.6545,14.04,0.05,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
ZTF J060018.79+475603.4 20260405.1545 14.04CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.68,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.79,0.05,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
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461135.6545,13.57,0.05,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
Gaia DR3 197994904265884544 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.66,0.05,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
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.71,0.05,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
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.8513+48.1175,2461135.6545,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.8513+48.1175 20260405.1545 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.31,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 970780295297033600,2461135.6545,13.23,0.05,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 970780295297033600 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053104.45+465119.1,2461135.6545,13.63,0.05,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
ASASSN-V J053104.45+465119.1 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.2817+44.3087,2461135.6545,13.49,0.05,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 J083.2817+44.3087 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.49,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.33,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192462196116236160,2461135.6545,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192462196116236160 20260405.1545 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.9406+46.9289,2461135.6545,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.9406+46.9289 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.8530+42.8735,2461135.6545,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.8530+42.8735 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.23,0.05,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
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6295+48.7004,2461135.6545,13.24,0.05,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 J084.6295+48.7004 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.0151+41.6769,2461135.6545,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.0151+41.6769 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2220+45.5909,2461135.6545,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.2220+45.5909 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.9297+43.1685,2461135.6545,13.29,0.05,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 J085.9297+43.1685 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.9718+42.7833,2461135.6545,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.9718+42.7833 20260405.1545 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196183179687428352,2461135.6545,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196183179687428352 20260405.1545 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.1430+48.5601,2461135.6545,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.1430+48.5601 20260405.1545 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 194772338765794816,2461135.6545,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 194772338765794816 20260405.1545 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195907447082573312,2461135.6545,12.76,0.05,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 195907447082573312 20260405.1545 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.1833+42.4993,2461135.6545,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.1833+42.4993 20260405.1545 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209400894295907712,2461135.6545,12.61,0.05,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 209400894295907712 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.5437+43.6538,2461135.6545,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J087.5437+43.6538 20260405.1545 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195913627537772416,2461135.6545,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 195913627537772416 20260405.1545 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J062013.27+433839.0,2461135.6545,11.79,0.05,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
ASASSN-V J062013.27+433839.0 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192332281946145280,2461135.6545,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192332281946145280 20260405.1545 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.2458+42.5740,2461135.6545,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.2458+42.5740 20260405.1545 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192716728762870272,2461135.6545,11.56,0.05,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 192716728762870272 20260405.1545 11.56CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196143842081588352,2461135.6545,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196143842081588352 20260405.1545 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211109329208390656,2461135.6545,12.25,0.05,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
Gaia DR3 211109329208390656 20260405.1545 12.25CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.2681+41.6489,2461135.6545,12.60,0.05,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
ATO J083.2681+41.6489 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192357020957523712,2461135.6545,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192357020957523712 20260405.1545 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195751385150686464,2461135.6545,12.59,0.05,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 195751385150686464 20260405.1545 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.41,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.8867+42.5604,2461135.6545,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J081.8867+42.5604 20260405.1545 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461135.6545,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3195+44.0466 20260405.1545 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196601268981151360,2461135.6545,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196601268981151360 20260405.1545 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5149+42.4644,2461135.6545,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5149+42.4644 20260405.1545 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211485843219678720,2461135.6545,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211485843219678720 20260405.1545 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 195999702979561088,2461135.6545,12.92,0.05,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 195999702979561088 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461135.6545,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.6351+48.1884 20260405.1545 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5805+44.4532,2461135.6545,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5805+44.4532 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.0691+46.8574,2461135.6545,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.0691+46.8574 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209517442528659072,2461135.6545,12.94,0.05,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
Gaia DR3 209517442528659072 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.2390+42.2966,2461135.6545,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.2390+42.2966 20260405.1545 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1509+45.4814,2461135.6545,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1509+45.4814 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4626+44.3866,2461135.6545,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.4626+44.3866 20260405.1545 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.1629+50.0440,2461135.6545,13.18,0.05,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
ATO J084.1629+50.0440 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 959056340249435648,2461135.6545,12.66,0.05,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 959056340249435648 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461135.6545,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197388553666998656 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5567+44.2856,2461135.6545,13.07,0.05,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
ATO J083.5567+44.2856 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.4601+41.5222,2461135.6545,13.26,0.05,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 J083.4601+41.5222 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192463089469495040,2461135.6545,13.07,0.05,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 192463089469495040 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461135.6545,13.12,0.05,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 196552271996570368 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.8798+49.8178,2461135.6545,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.8798+49.8178 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197725867514471040,2461135.6545,13.17,0.05,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 197725867514471040 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.34,0.05,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
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.6503+44.5028,2461135.6545,13.39,0.05,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 J084.6503+44.5028 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209360929625931648,2461135.6545,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209360929625931648 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210103654024515072,2461135.6545,13.44,0.05,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 210103654024515072 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053745.20+455814.5,2461135.6545,13.27,0.05,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
ASASSN-V J053745.20+455814.5 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.6264+42.0076,2461135.6545,13.45,0.05,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
ATO J083.6264+42.0076 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J091.0747+46.9169,2461135.6545,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J091.0747+46.9169 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2314+46.6988,2461135.6545,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2314+46.6988 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5381+48.6224,2461135.6545,13.32,0.05,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 J089.5381+48.6224 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.2884+47.3636,2461135.6545,13.47,0.05,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
ATO J090.2884+47.3636 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.8336+46.6637,2461135.6545,13.76,0.05,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
ATO J084.8336+46.6637 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.1489+47.1851,2461135.6545,13.66,0.05,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
ATO J086.1489+47.1851 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J081.6441+45.5735,2461135.6545,13.64,0.05,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 J081.6441+45.5735 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 193611907321181312,2461135.6545,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 193611907321181312 20260405.1545 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.2469+50.0543,2461135.6545,13.87,0.05,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
ATO J085.2469+50.0543 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.68,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J083.5258+43.9001,2461135.6545,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J083.5258+43.9001 20260405.1545 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4467+42.4827,2461135.6545,13.67,0.05,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 J086.4467+42.4827 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210650661059367936,2461135.6545,13.81,0.05,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
Gaia DR3 210650661059367936 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.80,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.8999+48.2678,2461135.6545,13.57,0.05,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 J089.8999+48.2678 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.0517+43.2060,2461135.6545,13.79,0.05,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 J084.0517+43.2060 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.69,0.05,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 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209410240146444416,2461135.6545,13.65,0.05,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
Gaia DR3 209410240146444416 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.9114+46.7779,2461135.6545,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.9114+46.7779 20260405.1545 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J082.5835+46.8115,2461135.6545,13.91,0.05,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 J082.5835+46.8115 20260405.1545 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196653667584324352,2461135.6545,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196653667584324352 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197321075438633984,2461135.6545,13.70,0.05,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
Gaia DR3 197321075438633984 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.2799+47.0618,2461135.6545,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.2799+47.0618 20260405.1545 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.5013+48.1338,2461135.6545,13.80,0.05,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 J085.5013+48.1338 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.8933+41.9608,2461135.6545,13.95,0.05,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
ATO J086.8933+41.9608 20260405.1545 13.95CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.4318+48.5650,2461135.6545,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J085.4318+48.5650 20260405.1545 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.94,0.05,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
target 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1759+48.7398,2461135.6545,13.70,0.05,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 J089.1759+48.7398 20260405.1545 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.99,0.05,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 20260405.1545 13.99CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210342484270003328,2461135.6545,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210342484270003328 20260405.1545 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.4564+48.9850,2461135.6545,13.99,0.05,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
ATO J087.4564+48.9850 20260405.1545 13.99CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4083+47.5260,2461135.6545,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.4083+47.5260 20260405.1545 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461135.6545,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260405.1545 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196584363989884800,2461135.6545,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196584363989884800 20260405.1545 13.90CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461135.65477061 05.04.2026 03:42:42.181 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18574
Objects passed selection criteria: 18536
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 16281.8
Average stars matched: 15875 (97.5018 %)
Memory usage VmPeak: 124184 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 4 22:47:24 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: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
First image: 2461061.71554414 21.01.2026 05:10:13.014 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Last image: 2461135.65477061 05.04.2026 03:42:42.181 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 383
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 80 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): 138310
Objects passed selection criteria: 137971
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 124088
Average stars matched: 119658 (96.4307 %)
Memory usage VmPeak: 1917392 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 4 22:50:03 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461135.65419916
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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits'
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:00.429 +46:00:18.65
Angular distance between the image centers 0.0368 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 05:59:57.911 +46:00:22.95
Angular distance between the image centers 0.0294 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 06:00:00.429 +46:00:18.65
Second-epoch second image center 05:59:57.911 +46:00:22.95
Angular distance between the image centers 0.00739 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.MbivKAno1K
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.ZDkxfSWzTY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits &> /tmp/tmp.JY6kzM2XmU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits &> /tmp/tmp.oZ8bYau7M7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 24266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.9190 to 102.4864 deg, Dec +39.9773 to +51.3461 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 77.9190 to 102.4864 deg, Dec 39.9773 to 51.3461 deg
Loaded 11816 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): 86 out of 101 total matches.
Matched with Tycho-2 101 out of 24266 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 23.040760
a=0.000000 b=1.000000 c=23.040760
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.2 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.6 pix fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
2.6 pix fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Limiting magnitude estimates:
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
15.4 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.9 mag. fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
14.9 mag. fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (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.MbivKAno1K (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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2260, passed=24266
Got 24266 stars (including 21982 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 24266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 417 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 363 matched stars entering correct_measured_positions(), 321 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.91"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 354 matched stars entering correct_measured_positions(), 9707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.36"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 406 matched stars entering correct_measured_positions(), 9733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 5.27"
WARNING: Accuracy estimation diagnostic: 405 matched stars entering correct_measured_positions(), 10903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 3.47"
Excluding outliers - 405 stars left (next iteration limit 389)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.ZDkxfSWzTY (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/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2222, passed=24282
Got 24282 stars (including 22031 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 24282 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
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...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 23377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.JY6kzM2XmU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1136, passed=17046
Got 17046 stars (including 15891 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 17046 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
WARNING: Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 16627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.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.oZ8bYau7M7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=17408
Got 17408 stars (including 16203 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 17408 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 17060 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 17059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
WARNING: Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 17059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31249_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 31249_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:27.53 +44:52:19.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31314_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 31314_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:22.97 +46:49:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31409_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 31409_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:14:58.96 +46:47:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31459_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 31459_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:13:22.53 +47:44:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31561_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 31561_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:33:38.46 +45:26:24.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Aur-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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat to cache
SExtractor catalog cache: saved Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits exists and is non-empty
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 06:00:00.429 +46:00:18.65
Angular distance between the image centers 0.0368 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:47.823 +46:00:35.63
Second-epoch image center 05:59:57.911 +46:00:22.95
Angular distance between the image centers 0.0294 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 06:00:00.429 +46:00:18.65
Second-epoch second image center 05:59:57.911 +46:00:22.95
Angular distance between the image centers 0.00739 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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.YEIdv58EGI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.3pkgDw9vaf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits &> /tmp/tmp.lxNTllGW7y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits &> /tmp/tmp.ZPBkOYTDQ6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
Found non-empty wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits and wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
The reference image (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits) and catalog (wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat) found
'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat' -> 'wcsmag.cat'
Read 170851 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 77.8948 to 102.5178 deg, Dec +39.9772 to +51.3479 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 77.8948 to 102.5178 deg, Dec 39.9772 to 51.3479 deg
Loaded 11844 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): 101 out of 140 total matches.
Matched with Tycho-2 140 out of 170851 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.801794
a=0.000000 b=1.000000 c=21.801794
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 318 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
2.0 pix Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
2.2 pix fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Limiting magnitude estimates:
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
14.5 mag. Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
14.0 mag. fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
14.0 mag. fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.YEIdv58EGI (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/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=46, blended=20120, passed=170805
Got 170805 stars (including 150422 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 170805 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 935.1'
Seting catalog search parameters based on the expected field of view 935.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012988 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010390 (37.4 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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 406 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 356 matched stars entering correct_measured_positions(), 310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.13"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 352 matched stars entering correct_measured_positions(), 60456 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.06"
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 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 442 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 410 matched stars entering correct_measured_positions(), 60493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.05"
WARNING: Accuracy estimation diagnostic: 409 matched stars entering correct_measured_positions(), 73193 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 4.14"
Excluding outliers - 409 stars left (next iteration limit 387)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.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.3pkgDw9vaf (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/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits' -> 'wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=20075, passed=170060
Got 170060 stars (including 149712 good ones) from the SExtractor catalog wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 170060 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 649 to 708 (Dec 40.0 to 51.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 166995 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.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.lxNTllGW7y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=11528, passed=121796
Got 121796 stars (including 110142 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 121796 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 118786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 118790 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
WARNING: Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 118790 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.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.ZPBkOYTDQ6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=39, blended=11986, passed=124300
Got 124300 stars (including 112190 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 124300 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 122143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 122144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 122144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.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_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_Aur-02-Q2b1x1_2026-01-20_23-10-59_20.00sec_-15.00C_LIGHT_0228.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-41-52_20.00sec_-4.90C_LIGHT_0046.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-04_CI_Aur-02-Q2b1x1_224503_TTUQ2b1x1_4691_BlHxOiRV/wcs_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out193161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out193171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193415.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196582.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 160s
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: 68s
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Considering the candidate 193161_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193161_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:56:15.01 +45:31:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.438 196920402231000832 089.06263104547 +45.51793777272 14.3071 13.6688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193171_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193171_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193178_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193178_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193180_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193180_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193182_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193182_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193183_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193183_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:50:38.21 +46:28:15.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 193198_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193198_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:56:51.00 +43:51:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.769 193527004408029696 089.21254198087 +43.85779592213 14.5463 13.8053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193203_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193203_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:18.21 +43:17:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.581 196241526818173952 085.07556648051 +43.28815022858 14.5880 13.7380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193204_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193204_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:59:22.80 +48:35:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.628 210242398647564672 089.84474307216 +48.59309551405 14.5051 13.8003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193216_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193216_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193217_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193217_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:26.10 +47:08:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.994 210575241433860096 084.10908187897 +47.13663121219 14.4334 13.5828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193219_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193219_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:12.74 +44:57:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193220_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193220_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193230_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193230_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193234_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193234_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:32:18.07 +47:26:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.040 209335920031032704 083.07526084274 +47.43459381099 14.4511 13.6188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193245_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193245_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:29:34.82 +44:55:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 5.173 965223466609101568 097.39549958770 +44.92987139218 14.1593 13.3933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193247_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193247_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:41:02.75 +45:28:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.528 197434806172188416 085.26166733685 +45.47032738571 14.3016 13.7120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193248_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193248_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:01:02.10 +48:38:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.020 969814580490083584 090.25833473206 +48.64796014011 14.3056 13.6622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193252_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193252_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:12.75 +44:18:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.658 197083787085249024 085.55409525404 +44.30225092962 14.2648 13.6264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193255_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193255_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:20.24 +41:55:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.336 193092800394897280 087.33390194821 +41.92263064796 14.2183 13.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193258_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193258_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193263_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193263_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193264_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193264_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193266_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193266_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:25.05 +45:43:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.140 209501087293588224 084.35462223877 +45.72979338931 14.0253 13.1241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193267_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193267_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193277_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193277_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193278_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193278_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:34.63 +45:49:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.947 209499815983191808 084.64501969201 +45.82343726759 14.0922 13.0991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193281_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193281_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193282_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193282_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193283_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193283_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193286_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193286_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:33:44.99 +45:05:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.789 207930087039286144 083.43731846808 +45.09819319577 14.4823 13.9288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193290_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193290_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193293_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193293_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:41:26.90 +43:07:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193294_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193294_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:27.45 +43:48:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.345 195611163059241088 083.61450272044 +43.80372310162 14.1797 13.5453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193302_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193302_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193304_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193304_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:50:48.16 +42:56:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.597 193384411494101120 087.70055001744 +42.94622564324 14.2469 13.6839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193305_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193305_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193307_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193307_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193308_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193308_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:52:59.28 +46:57:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.517 197994904265886976 088.24679455210 +46.95860760383 14.1710 13.4023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193310_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193310_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193314_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193314_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193315_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193315_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:00.40 +48:53:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193321_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193321_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:24:03.99 +44:40:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.345 959256898041674880 096.01653084857 +44.67501473517 13.9280 13.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193322_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193322_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:27.79 +42:06:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.032 194471862853689984 083.86558906076 +42.09992268831 14.2957 13.7190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193323_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193323_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:04.14 +43:45:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.494 195601336173976832 084.01706491764 +43.76183674387 14.2172 13.4494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193325_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193325_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 193327_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193327_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193328_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193328_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193331_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193331_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193332_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193332_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193334_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193334_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193346_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193346_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193349_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193349_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193354_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193354_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:40.50 +44:00:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193358_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193358_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193364_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193364_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193365_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193365_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:26.60 +45:10:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.329 197413400055078272 084.61129036399 +45.17145862977 14.2564 13.8011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193372_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193372_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:53:31.56 +49:45:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193377_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193377_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:56:29.62 +45:53:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.426 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193381_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193381_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:30:13.54 +44:13:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.326 207776400226843264 082.55694286433 +44.22264101995 14.0720 13.1129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193390_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193390_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193396_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193396_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:31.88 +44:07:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.310 197112614905505664 084.63250258375 +44.11974810978 13.9174 13.3239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193397_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193397_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:46.67 +47:09:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193398_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193398_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:56:59.29 +46:26:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.255 197790120225637760 089.24706019134 +46.44882066528 13.7375 13.0544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193401_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193401_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:29:09.83 +43:57:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193405_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193405_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:30.39 +43:50:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.232 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193406_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193406_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193407_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193407_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:30:25.74 +44:55:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193410_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193410_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:28:59.57 +42:20:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.457 958417966374346112 097.24824814175 +42.33868144266 13.2096 12.6635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193411_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193411_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:54.03 +47:59:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193415_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193415_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193420_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193420_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:24.13 +42:20:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193422_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193422_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193423_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193423_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:25.38 +41:59:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193425_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193425_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193426_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193426_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:34:44.76 +47:09:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.891 967180219349326464 098.68616762646 +47.15482328736 13.0175 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.891#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193431_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193431_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193433_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193433_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:16:36.43 +44:32:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.599 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193434_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193434_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:32.11 +41:33:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.083 194386856861482496 083.63319066159 +41.56110461880 13.5151 12.6425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193438_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193438_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:32:57.03 +44:10:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193441_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193441_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:28:11.79 +43:27:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193445_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193445_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193446_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193446_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193448_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193448_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:10.56 +43:24:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 0.716 195531963862337408 084.04372618786 +43.40619362145 13.2991 12.4824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193455_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193455_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:16.19 +45:33:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193457_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193457_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:11:13.07 +47:02:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193458_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193458_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:01.71 +46:28:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193459_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193459_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:31:36.62 +45:36:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.122 208183219528482560 082.90294986437 +45.60667736076 13.1671 12.2961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193461_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193461_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193469_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193469_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193470_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193470_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:42.42 +41:41:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193472_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193472_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:32:40.33 +42:27:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193474_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193474_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:53:23.97 +46:26:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.697 197734216930818048 088.35008467548 +46.44210108122 13.0058 12.2610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193475_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193475_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:41:57.62 +44:20:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.508 197084989676093184 085.49065431418 +44.34343392020 12.6672 11.5885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193477_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193477_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:41:47.93 +41:45:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193478_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193478_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:51:38.26 +48:20:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193479_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193479_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:23.57 +49:53:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193480_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193480_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193481_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193481_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:54:42.22 +43:39:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.591 193520201179972864 088.67569284427 +43.65050029424 12.3199 11.5214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193482_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193482_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:58:32.73 +44:49:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.621 196654320417663232 089.63653014033 +44.82054966257 12.4353 11.8337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193483_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193483_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:46.00 +43:34:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193484_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193484_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:09.05 +46:13:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193485_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193485_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:48:07.49 +45:19:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 0.584 197617561323923584 087.03135150238 +45.31853933119 12.1463 11.6118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193486_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193486_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:26:48.15 +43:44:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193488_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193488_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 193490_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193490_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:43:27.58 +42:19:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193597_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193597_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:28.49 +43:00:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193629_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193629_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:22.93 +46:49:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193837_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193837_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:45:42.93 +43:37:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193842_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193842_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:19.54 +42:40:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193899_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193899_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:11:34.58 +48:44:36.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193906_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193906_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:33:38.43 +45:26:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193917_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 193917_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:46:26.52 +47:55:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193971_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 193971_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194048_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194048_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:17.71 +45:03:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194102_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194102_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:32:51.89 +42:57:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194108_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194108_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:07.68 +44:53:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194113_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194113_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:02.90 +50:02:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194127_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194127_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:19:04.25 +47:21:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194165_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194165_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:37.54 +45:55:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194208_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194208_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:51.46 +48:19:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194243_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194243_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:43:17.32 +42:28:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194260_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194260_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:48:04.10 +43:19:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194294_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194294_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:23.84 +47:29:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194307_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194307_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194342_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194342_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:05:50.20 +44:39:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194361_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194361_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:30:40.86 +41:28:15.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194373_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194373_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194397_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194397_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:32.68 +43:42:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194424_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194424_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:43:52.78 +47:06:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194468_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194468_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:17.74 +42:18:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194474_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194474_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:47:16.22 +46:04:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194477_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194477_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:30:09.31 +46:12:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194494_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194494_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:50.36 +42:19:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.265 195370954129149312 081.96056057116 +42.32939550208 13.3071 12.4499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194531_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194531_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:46.10 +45:53:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194535_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194535_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:25.97 +48:47:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194537_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194537_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:31:06.99 +48:10:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194569_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194569_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:14.19 +50:00:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194575_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194575_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194580_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194580_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194589_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194589_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:40:28.28 +42:14:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194591_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194591_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:33:24.00 +43:46:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194606_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194606_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:30:11.29 +41:46:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194613_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194613_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:30:57.14 +43:05:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194615_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194615_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194638_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194638_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:26.18 +44:48:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194642_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194642_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194647_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194647_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:35.24 +44:15:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194654_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194654_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:46.56 +46:04:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194658_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194658_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:31:00.44 +42:54:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194670_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194670_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194673_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194673_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:46.25 +43:03:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194674_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194674_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:44.82 +44:40:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.609 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194689_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194689_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:43:06.54 +44:51:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194693_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194693_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:47:45.36 +50:03:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194718_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194718_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:24.47 +42:59:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194719_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194719_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:52:03.68 +49:32:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194726_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194726_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:22.11 +42:59:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194733_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194733_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:28:50.53 +44:16:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194740_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194740_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:32.69 +41:57:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194748_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194748_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194756_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194756_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:06.28 +45:12:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194784_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194784_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:02.67 +46:44:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194793_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194793_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:01:04.74 +50:00:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194795_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194795_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:29.91 +44:44:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194799_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194799_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:11:01.08 +47:29:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194821_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194821_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:44:39.87 +43:57:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194822_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194822_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:03.60 +46:04:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.115 208968026014384256 081.76535198396 +46.07821817677 13.5233 12.7276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194840_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194840_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194847_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194847_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194870_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194870_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:50.55 +49:49:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194879_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194879_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:17:34.76 +46:23:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194917_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194917_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:57.57 +42:25:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194919_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194919_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194941_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194941_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:31:17.72 +46:25:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194943_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194943_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194945_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194945_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:43:56.72 +47:43:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.857 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194958_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194958_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194965_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194965_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:26:13.45 +46:47:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194973_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 194973_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 194978_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 194978_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:46:39.79 +43:21:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.545 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195042_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195042_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:18.74 +47:12:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.327 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195045_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195045_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:52:21.21 +42:50:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195048_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195048_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195064_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195064_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:36:07.28 +47:47:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.521 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195078_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195078_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195108_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195108_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:00:13.95 +47:43:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195131_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195131_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195137_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195137_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195151_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195151_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:50.79 +48:07:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.144 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195153_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195153_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:41.40 +44:16:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195156_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195156_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195162_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195162_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:27.92 +47:51:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.449 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195186_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195186_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:45.36 +45:54:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.433 196999777523639936 089.43970142505 +45.91480103623 13.9429 13.4194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195191_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195191_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:30:42.56 +45:28:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195198_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195198_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:49:25.49 +42:20:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.556 193164474809048320 087.35669110624 +42.33491068620 13.9992 13.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195199_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195199_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195200_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195200_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195207_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195207_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195211_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195211_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195220_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195220_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:00.84 +46:20:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.059 208287501334038656 083.50390290064 +46.33909529807 14.0153 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195236_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195236_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195243_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195243_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:21.15 +42:12:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.604 194485228791887360 083.83941947095 +42.21584423136 13.9826 12.9019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195247_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195247_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:31:20.14 +45:58:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.420 208252729279086464 082.83335404737 +45.97527379616 13.9254 13.0817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195251_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195251_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:48:44.82 +49:34:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.081 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195255_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195255_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195259_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195259_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195260_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195260_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:53:58.77 +46:09:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195273_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195273_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195280_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195280_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:24.86 +49:14:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.598 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195290_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195290_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:53.90 +46:32:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.511 209184908981247744 081.97518253378 +46.54961465738 14.0914 13.2181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195292_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195292_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:59.93 +47:35:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.996 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195298_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195298_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:35:31.06 +48:04:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195301_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195301_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:16.20 +43:16:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195304_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195304_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:45:24.73 +43:50:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195306_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195306_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195327_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195327_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:23.57 +49:49:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.550 214254619657430144 084.84769115489 +49.82477197399 14.0502 13.3596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195353_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195353_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195358_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195358_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:41:40.18 +42:55:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195359_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195359_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:43.50 +41:40:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195400_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195400_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195401_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195401_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195412_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195412_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:50:06.52 +46:08:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195429_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195429_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:53:28.99 +46:52:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.647 197945941638985728 088.37080176482 +46.86831856952 13.9453 13.1591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195439_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195439_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:12:20.05 +50:12:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195442_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195442_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:28:36.09 +44:21:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195448_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195448_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:50:24.02 +41:41:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195453_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195453_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:11:51.69 +45:03:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.327 963207615120236544 092.96583890432 +45.05666831276 14.0648 13.4839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195472_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195472_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195475_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195475_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:15.67 +45:20:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195478_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195478_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:11.47 +42:50:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.249 192511364902195840 089.29695470380 +42.84027162771 14.0339 13.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195494_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195494_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:55.01 +44:13:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.864 207787635860868992 081.98001002011 +44.23068927629 14.0118 13.1106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195506_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195506_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195515_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195515_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195550_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195550_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195571_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195571_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:53:58.33 +42:30:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.987 192386845210042624 088.49355776279 +42.50729470844 14.1038 13.2843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195584_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195584_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:13:33.71 +48:03:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.275 969210708089081216 093.39001337563 +48.05522019758 14.0114 13.4390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195650_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195650_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:56:00.84 +49:05:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.422 210502639306225152 089.00335369221 +49.08957753130 14.0985 13.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195663_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195663_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195667_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195667_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:32:28.47 +41:32:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.812 194340608653387776 083.11828276699 +41.54734453710 14.2290 13.4809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195668_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195668_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:47:11.20 +46:03:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.743 197523351216767360 086.79557643499 +46.05504755708 14.1430 13.2999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195722_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195722_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195739_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195739_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195747_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195747_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195752_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195752_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:41:07.41 +47:58:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195759_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195759_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:17:15.27 +42:06:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195791_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195791_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195796_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195796_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:47.41 +45:58:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195850_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195850_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 195916_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195916_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195938_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 195938_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195939_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195939_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:08.67 +44:17:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.001 195826594321239040 083.53574128686 +44.28348556654 14.4393 13.6154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195973_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 195973_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:43:51.99 +41:39:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.102 192757792945027968 085.96660850387 +41.66113921297 14.5630 13.9268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196000_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196000_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196003_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196003_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196019_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196019_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196028_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196028_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:45.12 +44:19:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.672 197139690379212416 084.93820444258 +44.32014386784 14.4944 13.7284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196044_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196044_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196058_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196058_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196070_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196070_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:34:28.28 +41:57:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.740 194446093050327680 083.61786697562 +41.96324037214 14.3406 13.3995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196084_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196084_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:44:47.15 +46:28:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.204 209612206687131136 086.19689831834 +46.47272458834 14.4861 13.7429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196108_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196108_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196120_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196120_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196147_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196147_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196153_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196153_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196156_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196156_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196177_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196177_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196181_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196181_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196186_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196186_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196203_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196203_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196210_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196210_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:44:12.61 +41:54:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.322 192765077209505024 086.05332227939 +41.91528063423 14.6344 13.7936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196222_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196222_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196233_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196233_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:38:54.39 +43:44:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.188 197043586191465216 084.72697828945 +43.73626464419 14.7384 13.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196234_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196234_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196236_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196236_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:33:22.68 +45:21:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.245 207994550205149568 083.34478647209 +45.35922558133 14.6379 14.0318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196250_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196250_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:32:24.43 +42:36:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.103 194731343302441472 083.10214061917 +42.60061152598 14.3840 13.5368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196253_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196253_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196255_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196255_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:39:23.72 +48:22:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.478 210892278739539712 084.84907244679 +48.37243398973 14.7767 14.0675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196264_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196264_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:58:27.53 +43:46:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.532 193346821940150144 089.61512686000 +43.77366276940 14.6138 13.9693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196269_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196269_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196282_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196282_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:27:02.09 +46:15:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.455 208985313260690688 081.75929195173 +46.25217209926 14.8339 14.1927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196291_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196291_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196296_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196296_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196320_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196320_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:31.60 +41:47:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.729 192857917222804096 085.63183763419 +41.79599060573 14.3975 13.5331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196325_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196325_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:17.42 +47:02:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196331_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196331_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:31:30.65 +46:47:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.951 209095470581442176 082.87740269802 +46.78669992141 14.8449 14.1982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196336_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196336_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 196346_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196346_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:51:17.49 +48:38:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.233 210393066101070976 087.82317447496 +48.64291830688 14.5406 13.7761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196349_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196349_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196354_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196354_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196356_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196356_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196358_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196358_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:45:41.05 +48:34:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.730 210816103199445760 086.42134714368 +48.57123440831 14.8715 14.3053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196366_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196366_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196373_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196373_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:44:30.19 +47:32:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.997 209950065994494848 086.12619133731 +47.54710414041 14.7668 13.9588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196382_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196382_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:55:41.03 +43:20:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.889 193316413571991808 088.92112805465 +43.34226942073 14.8021 13.9780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196390_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196390_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:42:37.07 +42:58:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.257 195976819393890048 085.65451684002 +42.97941518346 14.5822 13.6169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196403_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196403_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196422_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196422_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:45:52.16 +44:26:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.769 196439816867899776 086.46762874449 +44.43992327227 14.7670 14.0003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196440_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196440_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196446_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196446_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196447_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196447_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:51:17.59 +42:37:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.890 193174232974513152 087.82360314860 +42.63264845655 14.8208 14.0661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196448_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196448_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196469_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196469_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196472_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196472_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196505_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196505_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:46:50.82 +46:54:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.915 209674981928902528 086.71240249685 +46.91581834305 14.7890 14.1581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196539_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196539_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196543_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196543_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:53:44.13 +43:57:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.420 193507621217635968 088.43409600159 +43.95602754150 15.0092 14.4070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196563_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196563_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196582_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
Preparing report for the candidate 196582_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
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Considering the candidate 196592_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196592_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:56:24.42 +42:43:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.389 192485698177107712 089.10159296932 +42.72801470474 14.8782 14.2704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196657_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 196657_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:55:18.10 +43:58:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.847 193587237029432704 088.82516235594 +43.97743555834 14.8197 13.9349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:59:44.18 +47:37:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123500_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 123500_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 75365_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 75365_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48194_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 48194_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:13:22.54 +47:44:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:57:24.03 +48:22:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 05:37:57.04 +44:41:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-04_22-42-42_20.00sec_-5.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:14:58.94 +46:47:45.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 235s
Prepared the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:59:03.25 +42:44:48.7
06:00:18.86 +47:56:02.8
05:52:56.68 +47:14:08.4
05:53:50.16 +48:42:12.8
05:53:04.93 +46:58:01.4
05:44:06.46 +47:04:02.0
05:56:42.44 +44:14:58.7
05:37:14.60 +47:38:54.6
05:34:14.18 +45:48:33.7
06:32:48.81 +42:55:22.7
05:47:24.47 +48:07:01.0
05:56:18.32 +42:39:03.6
06:22:08.96 +50:01:03.7
05:31:04.10 +46:51:16.5
05:33:07.77 +44:18:48.3
05:40:13.51 +48:11:29.8
05:37:50.80 +42:33:00.8
05:55:10.07 +42:25:14.6
05:51:45.79 +46:56:07.8
05:47:02.58 +44:49:00.1
05:48:30.25 +42:09:06.1
05:51:25.09 +42:52:19.5
05:32:55.48 +46:44:10.6
05:38:30.91 +48:42:00.9
05:32:03.43 +41:40:36.9
05:48:55.33 +45:35:43.7
05:43:43.05 +43:10:04.5
06:27:52.64 +42:46:55.5
06:18:26.42 +43:47:20.0
05:47:57.04 +44:02:17.4
06:00:35.31 +48:33:24.7
06:24:58.13 +42:35:45.6
05:35:49.11 +43:04:59.3
05:45:11.18 +42:07:49.6
05:37:57.12 +41:54:55.4
05:32:45.85 +42:29:56.9
05:31:27.69 +47:36:58.2
05:50:10.22 +43:38:46.8
05:38:24.35 +42:05:10.5
06:20:12.81 +43:38:52.9
05:50:23.58 +41:49:03.6
06:21:01.12 +42:34:37.7
05:48:33.27 +41:48:56.1
05:43:47.27 +43:32:40.8
05:48:15.12 +48:19:44.4
05:33:04.36 +41:38:37.2
05:52:45.77 +42:03:42.7
05:28:58.85 +43:48:26.9
06:12:10.27 +50:14:53.2
06:11:49.34 +45:03:15.6
05:27:51.09 +42:20:25.8
05:27:34.73 +42:32:45.4
05:37:16.33 +44:02:45.7
05:52:15.69 +44:44:13.2
05:34:04.42 +42:27:51.8
05:48:23.25 +49:46:56.4
05:37:44.81 +42:36:37.7
05:37:52.53 +43:02:32.2
06:02:32.06 +48:11:23.8
05:34:19.09 +44:27:46.0
05:40:16.09 +46:51:03.6
05:37:49.80 +45:56:18.7
05:52:55.16 +42:18:27.4
05:56:33.82 +45:29:09.4
05:45:50.43 +44:23:03.0
05:36:40.86 +50:02:57.7
06:25:57.49 +43:06:03.8
05:37:19.44 +44:51:38.2
05:34:15.72 +44:17:03.9
05:33:50.43 +41:31:21.3
05:54:37.63 +42:21:15.5
05:50:28.80 +44:11:35.9
06:26:29.72 +49:54:12.5
05:49:38.78 +47:49:48.0
05:39:33.76 +49:48:35.2
05:52:11.40 +46:15:47.5
05:46:44.52 +43:22:48.2
05:38:34.88 +44:30:48.2
05:30:47.13 +47:20:50.9
05:50:48.49 +47:35:34.8
05:37:41.40 +45:58:08.6
05:34:32.17 +42:00:23.8
06:04:15.68 +46:54:34.7
05:56:58.11 +46:41:26.9
05:58:09.52 +48:37:11.8
05:35:09.20 +46:30:56.2
06:01:02.25 +47:22:14.3
05:39:18.82 +46:40:23.7
05:44:39.76 +47:11:54.6
05:26:36.78 +45:34:11.6
05:55:36.76 +44:15:35.4
05:40:58.10 +50:02:31.4
06:00:34.71 +46:38:48.8
05:34:05.71 +43:53:41.1
05:45:48.68 +42:29:30.0
05:38:35.16 +47:30:20.1
05:34:45.15 +46:34:27.8
05:59:33.96 +48:16:25.8
05:36:13.11 +43:12:16.7
05:46:07.97 +44:11:58.5
05:33:17.92 +47:51:56.4
05:37:55.88 +43:03:20.2
06:03:36.25 +46:47:51.7
05:30:19.07 +46:48:41.4
05:58:07.37 +44:56:20.4
05:37:17.73 +44:28:42.3
05:37:07.11 +47:03:51.8
05:56:22.23 +48:25:41.1
05:41:57.74 +48:08:19.3
05:47:34.30 +41:57:38.4
05:41:41.45 +48:34:10.4
05:53:23.23 +50:05:49.5
05:56:44.55 +48:44:12.9
05:47:33.70 +49:04:01.4
05:49:05.48 +48:03:50.3
05:49:49.54 +48:59:05.9
05:45:41.68 +47:31:17.0
05:49:35.06 +42:10:24.8
05:52:45.30 +44:27:23.1
########### Completed Aur-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 ####
05:59:03.25 +42:44:48.7
06:00:18.86 +47:56:02.8
05:52:56.68 +47:14:08.4
05:53:50.16 +48:42:12.8
05:53:04.93 +46:58:01.4
05:44:06.46 +47:04:02.0
05:56:42.44 +44:14:58.7
05:37:14.60 +47:38:54.6
05:34:14.18 +45:48:33.7
06:32:48.81 +42:55:22.7
05:47:24.47 +48:07:01.0
05:56:18.32 +42:39:03.6
06:22:08.96 +50:01:03.7
05:31:04.10 +46:51:16.5
05:33:07.77 +44:18:48.3
05:40:13.51 +48:11:29.8
05:37:50.80 +42:33:00.8
05:55:10.07 +42:25:14.6
05:51:45.79 +46:56:07.8
05:47:02.58 +44:49:00.1
05:48:30.25 +42:09:06.1
05:51:25.09 +42:52:19.5
05:32:55.48 +46:44:10.6
05:38:30.91 +48:42:00.9
05:32:03.43 +41:40:36.9
05:48:55.33 +45:35:43.7
05:43:43.05 +43:10:04.5
06:27:52.64 +42:46:55.5
06:18:26.42 +43:47:20.0
05:47:57.04 +44:02:17.4
06:00:35.31 +48:33:24.7
06:24:58.13 +42:35:45.6
05:35:49.11 +43:04:59.3
05:45:11.18 +42:07:49.6
05:37:57.12 +41:54:55.4
05:32:45.85 +42:29:56.9
05:31:27.69 +47:36:58.2
05:50:10.22 +43:38:46.8
05:38:24.35 +42:05:10.5
06:20:12.81 +43:38:52.9
05:50:23.58 +41:49:03.6
06:21:01.12 +42:34:37.7
05:48:33.27 +41:48:56.1
05:43:47.27 +43:32:40.8
05:48:15.12 +48:19:44.4
05:33:04.36 +41:38:37.2
05:52:45.77 +42:03:42.7
05:28:58.85 +43:48:26.9
06:12:10.27 +50:14:53.2
06:11:49.34 +45:03:15.6
05:27:51.09 +42:20:25.8
05:27:34.73 +42:32:45.4
05:37:16.33 +44:02:45.7
05:52:15.69 +44:44:13.2
05:34:04.42 +42:27:51.8
05:48:23.25 +49:46:56.4
05:37:44.81 +42:36:37.7
05:37:52.53 +43:02:32.2
06:02:32.06 +48:11:23.8
05:34:19.09 +44:27:46.0
05:40:16.09 +46:51:03.6
05:37:49.80 +45:56:18.7
05:52:55.16 +42:18:27.4
05:56:33.82 +45:29:09.4
05:45:50.43 +44:23:03.0
05:36:40.86 +50:02:57.7
06:25:57.49 +43:06:03.8
05:37:19.44 +44:51:38.2
05:34:15.72 +44:17:03.9
05:33:50.43 +41:31:21.3
05:54:37.63 +42:21:15.5
05:50:28.80 +44:11:35.9
06:26:29.72 +49:54:12.5
05:49:38.78 +47:49:48.0
05:39:33.76 +49:48:35.2
05:52:11.40 +46:15:47.5
05:46:44.52 +43:22:48.2
05:38:34.88 +44:30:48.2
05:30:47.13 +47:20:50.9
05:50:48.49 +47:35:34.8
05:37:41.40 +45:58:08.6
05:34:32.17 +42:00:23.8
06:04:15.68 +46:54:34.7
05:56:58.11 +46:41:26.9
05:58:09.52 +48:37:11.8
05:35:09.20 +46:30:56.2
06:01:02.25 +47:22:14.3
05:39:18.82 +46:40:23.7
05:44:39.76 +47:11:54.6
05:26:36.78 +45:34:11.6
05:55:36.76 +44:15:35.4
05:40:58.10 +50:02:31.4
06:00:34.71 +46:38:48.8
05:34:05.71 +43:53:41.1
05:45:48.68 +42:29:30.0
05:38:35.16 +47:30:20.1
05:34:45.15 +46:34:27.8
05:59:33.96 +48:16:25.8
05:36:13.11 +43:12:16.7
05:46:07.97 +44:11:58.5
05:33:17.92 +47:51:56.4
05:37:55.88 +43:03:20.2
06:03:36.25 +46:47:51.7
05:30:19.07 +46:48:41.4
05:58:07.37 +44:56:20.4
05:37:17.73 +44:28:42.3
05:37:07.11 +47:03:51.8
05:56:22.23 +48:25:41.1
05:41:57.74 +48:08:19.3
05:47:34.30 +41:57:38.4
05:41:41.45 +48:34:10.4
05:53:23.23 +50:05:49.5
05:56:44.55 +48:44:12.9
05:47:33.70 +49:04:01.4
05:49:05.48 +48:03:50.3
05:49:49.54 +48:59:05.9
05:45:41.68 +47:31:17.0
05:49:35.06 +42:10:24.8
05:52:45.30 +44:27:23.1
###################################################################################
05:59:03.25 +42:44:48.7 -- not an asteroid (will add it to exclusion list)
06:00:18.86 +47:56:02.8 -- not an asteroid (will add it to exclusion list)
05:52:56.68 +47:14:08.4 -- not an asteroid (will add it to exclusion list)
05:53:50.16 +48:42:12.8 -- not an asteroid (will add it to exclusion list)
05:53:04.93 +46:58:01.4 -- not an asteroid (will add it to exclusion list)
05:44:06.46 +47:04:02.0 -- not an asteroid (will add it to exclusion list)
05:56:42.44 +44:14:58.7 -- not an asteroid (will add it to exclusion list)
05:37:14.60 +47:38:54.6 -- not an asteroid (will add it to exclusion list)
05:34:14.18 +45:48:33.7 -- not an asteroid (will add it to exclusion list)
06:32:48.81 +42:55:22.7 -- not an asteroid (will add it to exclusion list)
05:47:24.47 +48:07:01.0 -- not an asteroid (will add it to exclusion list)
05:56:18.32 +42:39:03.6 -- not an asteroid (will add it to exclusion list)
06:22:08.96 +50:01:03.7 -- not an asteroid (will add it to exclusion list)
05:31:04.10 +46:51:16.5 -- not an asteroid (will add it to exclusion list)
05:33:07.77 +44:18:48.3 -- not an asteroid (will add it to exclusion list)
05:40:13.51 +48:11:29.8 -- not an asteroid (will add it to exclusion list)
05:37:50.80 +42:33:00.8 -- not an asteroid (will add it to exclusion list)
05:55:10.07 +42:25:14.6 -- not an asteroid (will add it to exclusion list)
05:51:45.79 +46:56:07.8 -- not an asteroid (will add it to exclusion list)
05:47:02.58 +44:49:00.1 -- not an asteroid (will add it to exclusion list)
05:48:30.25 +42:09:06.1 -- not an asteroid (will add it to exclusion list)
05:51:25.09 +42:52:19.5 -- not an asteroid (will add it to exclusion list)
05:32:55.48 +46:44:10.6 -- not an asteroid (will add it to exclusion list)
05:38:30.91 +48:42:00.9 -- not an asteroid (will add it to exclusion list)
05:32:03.43 +41:40:36.9 -- not an asteroid (will add it to exclusion list)
05:48:55.33 +45:35:43.7 -- not an asteroid (will add it to exclusion list)
05:43:43.05 +43:10:04.5 -- not an asteroid (will add it to exclusion list)
06:27:52.64 +42:46:55.5 -- not an asteroid (will add it to exclusion list)
06:18:26.42 +43:47:20.0 -- not an asteroid (will add it to exclusion list)
05:47:57.04 +44:02:17.4 -- not an asteroid (will add it to exclusion list)
06:00:35.31 +48:33:24.7 -- not an asteroid (will add it to exclusion list)
06:24:58.13 +42:35:45.6 -- not an asteroid (will add it to exclusion list)
05:35:49.11 +43:04:59.3 -- not an asteroid (will add it to exclusion list)
05:45:11.18 +42:07:49.6 -- not an asteroid (will add it to exclusion list)
05:37:57.12 +41:54:55.4 -- not an asteroid (will add it to exclusion list)
05:32:45.85 +42:29:56.9 -- not an asteroid (will add it to exclusion list)
05:31:27.69 +47:36:58.2 -- not an asteroid (will add it to exclusion list)
05:50:10.22 +43:38:46.8 -- not an asteroid (will add it to exclusion list)
05:38:24.35 +42:05:10.5 -- not an asteroid (will add it to exclusion list)
06:20:12.81 +43:38:52.9 -- not an asteroid (will add it to exclusion list)
05:50:23.58 +41:49:03.6 -- not an asteroid (will add it to exclusion list)
06:21:01.12 +42:34:37.7 -- not an asteroid (will add it to exclusion list)
05:48:33.27 +41:48:56.1 -- not an asteroid (will add it to exclusion list)
05:43:47.27 +43:32:40.8 -- not an asteroid (will add it to exclusion list)
05:48:15.12 +48:19:44.4 -- not an asteroid (will add it to exclusion list)
05:33:04.36 +41:38:37.2 -- not an asteroid (will add it to exclusion list)
05:52:45.77 +42:03:42.7 -- not an asteroid (will add it to exclusion list)
05:28:58.85 +43:48:26.9 -- not an asteroid (will add it to exclusion list)
06:12:10.27 +50:14:53.2 -- not an asteroid (will add it to exclusion list)
06:11:49.34 +45:03:15.6 -- not an asteroid (will add it to exclusion list)
05:27:51.09 +42:20:25.8 -- not an asteroid (will add it to exclusion list)
05:27:34.73 +42:32:45.4 -- not an asteroid (will add it to exclusion list)
05:37:16.33 +44:02:45.7 -- not an asteroid (will add it to exclusion list)
05:52:15.69 +44:44:13.2 -- not an asteroid (will add it to exclusion list)
05:34:04.42 +42:27:51.8 -- not an asteroid (will add it to exclusion list)
05:48:23.25 +49:46:56.4 -- not an asteroid (will add it to exclusion list)
05:37:44.81 +42:36:37.7 -- not an asteroid (will add it to exclusion list)
05:37:52.53 +43:02:32.2 -- not an asteroid (will add it to exclusion list)
06:02:32.06 +48:11:23.8 -- not an asteroid (will add it to exclusion list)
05:34:19.09 +44:27:46.0 -- not an asteroid (will add it to exclusion list)
05:40:16.09 +46:51:03.6 -- not an asteroid (will add it to exclusion list)
05:37:49.80 +45:56:18.7 -- not an asteroid (will add it to exclusion list)
05:52:55.16 +42:18:27.4 -- not an asteroid (will add it to exclusion list)
05:56:33.82 +45:29:09.4 -- not an asteroid (will add it to exclusion list)
05:45:50.43 +44:23:03.0 -- not an asteroid (will add it to exclusion list)
05:36:40.86 +50:02:57.7 -- not an asteroid (will add it to exclusion list)
06:25:57.49 +43:06:03.8 -- not an asteroid (will add it to exclusion list)
05:37:19.44 +44:51:38.2 -- not an asteroid (will add it to exclusion list)
05:34:15.72 +44:17:03.9 -- not an asteroid (will add it to exclusion list)
05:33:50.43 +41:31:21.3 -- not an asteroid (will add it to exclusion list)
05:54:37.63 +42:21:15.5 -- not an asteroid (will add it to exclusion list)
05:50:28.80 +44:11:35.9 -- not an asteroid (will add it to exclusion list)
06:26:29.72 +49:54:12.5 -- not an asteroid (will add it to exclusion list)
05:49:38.78 +47:49:48.0 -- not an asteroid (will add it to exclusion list)
05:39:33.76 +49:48:35.2 -- not an asteroid (will add it to exclusion list)
05:52:11.40 +46:15:47.5 -- not an asteroid (will add it to exclusion list)
05:46:44.52 +43:22:48.2 -- not an asteroid (will add it to exclusion list)
05:38:34.88 +44:30:48.2 -- not an asteroid (will add it to exclusion list)
05:30:47.13 +47:20:50.9 -- not an asteroid (will add it to exclusion list)
05:50:48.49 +47:35:34.8 -- not an asteroid (will add it to exclusion list)
05:37:41.40 +45:58:08.6 -- not an asteroid (will add it to exclusion list)
05:34:32.17 +42:00:23.8 -- not an asteroid (will add it to exclusion list)
06:04:15.68 +46:54:34.7 -- not an asteroid (will add it to exclusion list)
05:56:58.11 +46:41:26.9 -- not an asteroid (will add it to exclusion list)
05:58:09.52 +48:37:11.8 -- not an asteroid (will add it to exclusion list)
05:35:09.20 +46:30:56.2 -- not an asteroid (will add it to exclusion list)
06:01:02.25 +47:22:14.3 -- not an asteroid (will add it to exclusion list)
05:39:18.82 +46:40:23.7 -- not an asteroid (will add it to exclusion list)
05:44:39.76 +47:11:54.6 -- not an asteroid (will add it to exclusion list)
05:26:36.78 +45:34:11.6 -- not an asteroid (will add it to exclusion list)
05:55:36.76 +44:15:35.4 -- not an asteroid (will add it to exclusion list)
05:40:58.10 +50:02:31.4 -- not an asteroid (will add it to exclusion list)
06:00:34.71 +46:38:48.8 -- not an asteroid (will add it to exclusion list)
05:34:05.71 +43:53:41.1 -- not an asteroid (will add it to exclusion list)
05:45:48.68 +42:29:30.0 -- not an asteroid (will add it to exclusion list)
05:38:35.16 +47:30:20.1 -- not an asteroid (will add it to exclusion list)
05:34:45.15 +46:34:27.8 -- not an asteroid (will add it to exclusion list)
05:59:33.96 +48:16:25.8 -- not an asteroid (will add it to exclusion list)
05:36:13.11 +43:12:16.7 -- not an asteroid (will add it to exclusion list)
05:46:07.97 +44:11:58.5 -- not an asteroid (will add it to exclusion list)
05:33:17.92 +47:51:56.4 -- not an asteroid (will add it to exclusion list)
05:37:55.88 +43:03:20.2 -- not an asteroid (will add it to exclusion list)
06:03:36.25 +46:47:51.7 -- not an asteroid (will add it to exclusion list)
05:30:19.07 +46:48:41.4 -- not an asteroid (will add it to exclusion list)
05:58:07.37 +44:56:20.4 -- not an asteroid (will add it to exclusion list)
05:37:17.73 +44:28:42.3 -- not an asteroid (will add it to exclusion list)
05:37:07.11 +47:03:51.8 -- not an asteroid (will add it to exclusion list)
05:56:22.23 +48:25:41.1 -- not an asteroid (will add it to exclusion list)
05:41:57.74 +48:08:19.3 -- not an asteroid (will add it to exclusion list)
05:47:34.30 +41:57:38.4 -- not an asteroid (will add it to exclusion list)
05:41:41.45 +48:34:10.4 -- not an asteroid (will add it to exclusion list)
05:53:23.23 +50:05:49.5 -- not an asteroid (will add it to exclusion list)
05:56:44.55 +48:44:12.9 -- not an asteroid (will add it to exclusion list)
05:47:33.70 +49:04:01.4 -- not an asteroid (will add it to exclusion list)
05:49:05.48 +48:03:50.3 -- not an asteroid (will add it to exclusion list)
05:49:49.54 +48:59:05.9 -- not an asteroid (will add it to exclusion list)
05:45:41.68 +47:31:17.0 -- not an asteroid (will add it to exclusion list)
05:49:35.06 +42:10:24.8 -- not an asteroid (will add it to exclusion list)
05:52:45.30 +44:27:23.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:26:36.78 +45:34:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:34.73 +42:32:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:51.09 +42:20:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:58.85 +43:48:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:19.07 +46:48:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:47.13 +47:20:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:04.10 +46:51:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:27.69 +47:36:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:03.43 +41:40:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:45.85 +42:29:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:55.48 +46:44:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:04.36 +41:38:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:07.77 +44:18:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:17.92 +47:51:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:50.43 +41:31:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:04.42 +42:27:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:05.71 +43:53:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:14.18 +45:48:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:15.72 +44:17:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:19.09 +44:27:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:32.17 +42:00:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:45.15 +46:34:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:09.20 +46:30:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:49.11 +43:04:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:13.11 +43:12:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:40.86 +50:02:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:07.11 +47:03:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:14.60 +47:38:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.33 +44:02:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:17.73 +44:28:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.44 +44:51:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.40 +45:58:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:44.81 +42:36:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:49.80 +45:56:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:50.80 +42:33:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:52.53 +43:02:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:55.88 +43:03:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:57.12 +41:54:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:24.35 +42:05:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:30.91 +48:42:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:34.88 +44:30:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:35.16 +47:30:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:18.82 +46:40:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:33.76 +49:48:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:13.51 +48:11:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:16.09 +46:51:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:58.10 +50:02:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:41.45 +48:34:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:57.74 +48:08:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:43.05 +43:10:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:47.27 +43:32:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:06.46 +47:04:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:39.76 +47:11:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:11.18 +42:07:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:41.68 +47:31:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:48.68 +42:29:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.43 +44:23:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:07.97 +44:11:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:44.52 +43:22:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:02.58 +44:49:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:24.47 +48:07:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:33.70 +49:04:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:34.30 +41:57:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:57.04 +44:02:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:15.12 +48:19:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.25 +49:46:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:30.25 +42:09:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:33.27 +41:48:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:55.33 +45:35:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:05.48 +48:03:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:35.06 +42:10:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:38.78 +47:49:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:49.54 +48:59:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.22 +43:38:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:23.58 +41:49:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.80 +44:11:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:48.49 +47:35:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:25.09 +42:52:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:45.79 +46:56:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:11.40 +46:15:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:15.69 +44:44:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:45.30 +44:27:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:45.77 +42:03:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:55.16 +42:18:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:56.68 +47:14:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.93 +46:58:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:23.23 +50:05:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:50.16 +48:42:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:37.63 +42:21:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:10.07 +42:25:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:36.76 +44:15:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:18.32 +42:39:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:22.23 +48:25:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.82 +45:29:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:42.44 +44:14:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:44.55 +48:44:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:58.11 +46:41:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:07.37 +44:56:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.52 +48:37:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:03.25 +42:44:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:33.96 +48:16:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:18.86 +47:56:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:34.71 +46:38:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:35.31 +48:33:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:02.25 +47:22:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.06 +48:11:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:36.25 +46:47:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:15.68 +46:54:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:49.34 +45:03:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.27 +50:14:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:18:26.42 +43:47:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:12.81 +43:38:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:01.12 +42:34:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:08.96 +50:01:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:58.13 +42:35:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:57.49 +43:06:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.72 +49:54:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:52.64 +42:46:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:48.81 +42:55:22.7 -- 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)
05:26:36.78 +45:34:11.6 -- not a known variable star
05:27:34.73 +42:32:45.4 -- not a known variable star
05:27:51.09 +42:20:25.8 -- not a known variable star
05:28:58.85 +43:48:26.9 -- not a known variable star
05:30:19.07 +46:48:41.4 -- not a known variable star
05:30:47.13 +47:20:50.9 -- not a known variable star
05:31:04.10 +46:51:16.5 -- a known variable star
05:31:27.69 +47:36:58.2 -- a known variable star
05:32:03.43 +41:40:36.9 -- not a known variable star
05:32:45.85 +42:29:56.9 -- not a known variable star
05:32:55.48 +46:44:10.6 -- not a known variable star
05:33:04.36 +41:38:37.2 -- not a known variable star
05:33:07.77 +44:18:48.3 -- not a known variable star
05:33:17.92 +47:51:56.4 -- not a known variable star
05:33:50.43 +41:31:21.3 -- not a known variable star
05:34:04.42 +42:27:51.8 -- not a known variable star
05:34:05.71 +43:53:41.1 -- not a known variable star
05:34:14.18 +45:48:33.7 -- not a known variable star
05:34:15.72 +44:17:03.9 -- not a known variable star
05:34:19.09 +44:27:46.0 -- not a known variable star
05:34:32.17 +42:00:23.8 -- not a known variable star
05:34:45.15 +46:34:27.8 -- not a known variable star
05:35:09.20 +46:30:56.2 -- not a known variable star
05:35:49.11 +43:04:59.3 -- a known variable star
05:36:13.11 +43:12:16.7 -- not a known variable star
05:36:40.86 +50:02:57.7 -- not a known variable star
05:37:07.11 +47:03:51.8 -- not a known variable star
05:37:14.60 +47:38:54.6 -- not a known variable star
05:37:16.33 +44:02:45.7 -- not a known variable star
05:37:17.73 +44:28:42.3 -- a known variable star
05:37:19.44 +44:51:38.2 -- not a known variable star
05:37:41.40 +45:58:08.6 -- not a known variable star
05:37:44.81 +42:36:37.7 -- a known variable star
05:37:49.80 +45:56:18.7 -- not a known variable star
05:37:50.80 +42:33:00.8 -- not a known variable star
05:37:52.53 +43:02:32.2 -- not a known variable star
05:37:55.88 +43:03:20.2 -- not a known variable star
05:37:57.12 +41:54:55.4 -- a known variable star
05:38:24.35 +42:05:10.5 -- a known variable star
05:38:30.91 +48:42:00.9 -- not a known variable star
05:38:34.88 +44:30:48.2 -- not a known variable star
05:38:35.16 +47:30:20.1 -- a known variable star
05:39:18.82 +46:40:23.7 -- not a known variable star
05:39:33.76 +49:48:35.2 -- not a known variable star
05:40:13.51 +48:11:29.8 -- not a known variable star
05:40:16.09 +46:51:03.6 -- not a known variable star
05:40:58.10 +50:02:31.4 -- not a known variable star
05:41:41.45 +48:34:10.4 -- not a known variable star
05:41:57.74 +48:08:19.3 -- not a known variable star
05:43:43.05 +43:10:04.5 -- not a known variable star
05:43:47.27 +43:32:40.8 -- not a known variable star
05:44:06.46 +47:04:02.0 -- not a known variable star
05:44:39.76 +47:11:54.6 -- not a known variable star
05:45:11.18 +42:07:49.6 -- not a known variable star
05:45:41.68 +47:31:17.0 -- not a known variable star
05:45:48.68 +42:29:30.0 -- not a known variable star
05:45:50.43 +44:23:03.0 -- not a known variable star
05:46:07.97 +44:11:58.5 -- not a known variable star
05:46:44.52 +43:22:48.2 -- not a known variable star
05:47:02.58 +44:49:00.1 -- not a known variable star
05:47:24.47 +48:07:01.0 -- not a known variable star
05:47:33.70 +49:04:01.4 -- not a known variable star
05:47:34.30 +41:57:38.4 -- not a known variable star
05:47:57.04 +44:02:17.4 -- a known variable star
05:48:15.12 +48:19:44.4 -- not a known variable star
05:48:23.25 +49:46:56.4 -- not a known variable star
05:48:30.25 +42:09:06.1 -- not a known variable star
05:48:33.27 +41:48:56.1 -- not a known variable star
05:48:55.33 +45:35:43.7 -- not a known variable star
05:49:05.48 +48:03:50.3 -- not a known variable star
05:49:35.06 +42:10:24.8 -- not a known variable star
05:49:38.78 +47:49:48.0 -- not a known variable star
05:49:49.54 +48:59:05.9 -- not a known variable star
05:50:10.22 +43:38:46.8 -- not a known variable star
05:50:23.58 +41:49:03.6 -- not a known variable star
05:50:28.80 +44:11:35.9 -- a known variable star
05:50:48.49 +47:35:34.8 -- a known variable star
05:51:25.09 +42:52:19.5 -- not a known variable star
05:51:45.79 +46:56:07.8 -- not a known variable star
05:52:11.40 +46:15:47.5 -- not a known variable star
05:52:15.69 +44:44:13.2 -- not a known variable star
05:52:45.30 +44:27:23.1 -- not a known variable star
05:52:45.77 +42:03:42.7 -- not a known variable star
05:52:55.16 +42:18:27.4 -- not a known variable star
05:52:56.68 +47:14:08.4 -- not a known variable star
05:53:04.93 +46:58:01.4 -- not a known variable star
05:53:23.23 +50:05:49.5 -- not a known variable star
05:53:50.16 +48:42:12.8 -- not a known variable star
05:54:37.63 +42:21:15.5 -- a known variable star
05:55:10.07 +42:25:14.6 -- a known variable star
05:55:36.76 +44:15:35.4 -- a known variable star
05:56:18.32 +42:39:03.6 -- not a known variable star
05:56:22.23 +48:25:41.1 -- not a known variable star
05:56:33.82 +45:29:09.4 -- not a known variable star
05:56:42.44 +44:14:58.7 -- not a known variable star
05:56:44.55 +48:44:12.9 -- not a known variable star
05:56:58.11 +46:41:26.9 -- not a known variable star
05:58:07.37 +44:56:20.4 -- a known variable star
05:58:09.52 +48:37:11.8 -- not a known variable star
05:59:03.25 +42:44:48.7 -- not a known variable star
05:59:33.96 +48:16:25.8 -- not a known variable star
06:00:18.86 +47:56:02.8 -- a known variable star
06:00:34.71 +46:38:48.8 -- not a known variable star
06:00:35.31 +48:33:24.7 -- not a known variable star
06:01:02.25 +47:22:14.3 -- not a known variable star
06:02:32.06 +48:11:23.8 -- not a known variable star
06:03:36.25 +46:47:51.7 -- not a known variable star
06:04:15.68 +46:54:34.7 -- not a known variable star
06:11:49.34 +45:03:15.6 -- not a known variable star
06:12:10.27 +50:14:53.2 -- not a known variable star
06:18:26.42 +43:47:20.0 -- not a known variable star
06:20:12.81 +43:38:52.9 -- a known variable star
06:21:01.12 +42:34:37.7 -- not a known variable star
06:22:08.96 +50:01:03.7 -- a known variable star
06:24:58.13 +42:35:45.6 -- not a known variable star
06:25:57.49 +43:06:03.8 -- a known variable star
06:26:29.72 +49:54:12.5 -- not a known variable star
06:27:52.64 +42:46:55.5 -- not a known variable star
06:32:48.81 +42:55:22.7 -- not a known variable star
Found 100 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
119 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 119 (excluding asteroids and hot pixels, 100 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461135.65419916 -observatory V36
23:16:06.66 -06:45:07.6 Mercury (0.3mag)
02:16:35.63 +13:23:27.9 Venus (-3.9mag)
23:46:56.00 -02:32:09.9 Mars (1.2mag)
07:08:21.17 +22:52:58.8 Jupiter (-2.2mag)
00:24:17.26 +00:18:13.6 Saturn (0.9mag)
03:45:31.49 +19:40:26.9 Uranus (5.8mag)
00:09:23.26 -00:24:34.5 Neptune (7.8mag)
20:33:10.23 -22:52:31.1 Pluto (14.5mag)
15:06:36.13 -22:52:04.2 Moon (-11.8mag)
-rw-r--r-- 1 apache apache 362 Apr 4 22:47 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461135.65419916:
07:08:13.98 +22:53:13.9 Io (5.7mag)
07:08:19.99 +22:53:04.1 Europa (5.8mag)
07:08:02.05 +22:53:38.9 Ganymede (5.3mag)
07:08:01.42 +22:53:28.0 Callisto (6.5mag)
07:12:06.09 +22:46:02.0 Himalia (15.3mag)
07:08:24.86 +22:52:49.8 Thebe (16.2mag)
07:12:02.24 +23:14:33.7 Elara (17.2mag)
07:06:29.76 +23:38:39.9 Pasiphae (17.3mag)
07:16:54.15 +22:49:46.9 Carme (18.4mag)
00:24:09.11 +00:18:22.6 Titan (8.8mag)
00:24:19.21 +00:18:27.4 Rhea (10.1mag)
00:24:20.22 +00:19:53.9 Iapetus (11.5mag)
00:24:15.27 +00:18:05.9 Hyperion (14.8mag)
00:26:02.21 +00:28:08.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 4 22:47 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461135.65419916:
14:41:05.40 -07:20:09.3 JWST
20:17:42.80 -08:05:21.9 Chandra
16:59:35.65 -51:09:00.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 4 22:47 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461135.65419916 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:46:30.30 -28:10:53.7 14.0mag P/2010 H2 (Vales)
04:59:25.99 -70:12:06.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:24.15 +31:22:12.9 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.53 +09:14:38.8 17.6mag C/2021 G2 (ATLAS)
23:07:00.98 +28:50:01.5 17.0mag C/2022 E2 (ATLAS)
04:16:49.71 +25:44:04.5 15.9mag C/2022 N2 (PANSTARRS)
09:01:46.29 +31:53:16.6 16.1mag C/2022 QE78 (ATLAS)
08:29:55.52 -01:21:06.4 17.3mag C/2022 R6 (PANSTARRS)
18:55:43.60 +17:36:17.4 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:45.92 -11:40:27.5 17.6mag P/2023 B1 (PANSTARRS)
09:13:28.24 -13:40:47.8 17.5mag C/2023 F3 (ATLAS)
21:42:13.69 +62:19:11.7 17.5mag C/2023 H5 (Lemmon)
19:27:01.42 -03:35:57.9 14.3mag C/2023 R1 (PANSTARRS)
21:42:51.45 +84:28:56.5 17.8mag C/2023 X2 (Lemmon)
06:14:19.94 +63:35:39.6 17.0mag C/2024 A1 (ATLAS)
04:48:32.95 +14:05:24.0 10.3mag C/2024 E1 (Wierzchos)
16:25:39.38 +04:36:26.6 17.4mag C/2024 G6 (ATLAS)
20:17:08.51 +12:25:08.3 14.7mag C/2024 J3 (ATLAS)
03:16:53.05 -24:05:27.8 16.4mag C/2024 T5 (ATLAS)
05:07:54.17 +48:07:05.8 17.7mag C/2025 J1 (Borisov)
14:23:10.86 +36:19:29.2 14.7mag C/2025 L1 (ATLAS)
03:08:51.94 -24:36:07.8 17.7mag C/2025 Q3 (ATLAS)
22:51:03.82 +19:49:44.9 10.3mag C/2025 R3 (PANSTARRS)
12:58:50.50 +02:19:26.9 17.5mag C/2025 Y1 (ATLAS)
01:09:00.24 +05:17:36.4 3.9mag C/2026 A1 (MAPS)
23:27:38.58 +35:00:43.6 14.2mag C/2026 B2 (Sun-Gao)
18:21:45.60 -10:16:00.3 12.5mag 10P/Tempel
15:14:06.46 +04:11:35.3 13.0mag 24P/Schaumasse
11:06:07.61 -01:54:06.7 15.7mag 29P/Schwassmann-Wachmann
17:56:08.83 -10:02:07.2 17.7mag 40P/Vaisala
10:39:08.37 -05:02:44.9 16.7mag 43P/Wolf-Harrington
01:31:57.70 +15:36:53.3 17.1mag 47P/Ashbrook-Jackson
06:51:34.94 +39:17:42.5 17.1mag 63P/Wild
23:14:55.80 -12:47:07.6 15.7mag 65P/Gunn
03:35:03.24 +17:20:53.7 15.8mag 76P/West-Kohoutek-Ikemura
00:41:49.83 +06:04:41.1 14.5mag 78P/Gehrels
22:29:13.80 -12:34:17.4 14.5mag 88P/Howell
01:40:21.59 +17:39:12.3 15.1mag 93P/Lovas
04:35:07.00 +31:39:54.5 16.3mag 123P/West-Hartley
08:16:59.38 +43:22:11.1 16.2mag 124P/Mrkos
02:16:39.18 +13:08:13.6 16.4mag 128P/Shoemaker-Holt
02:26:23.33 +13:07:02.8 17.5mag 131P/Mueller
00:30:44.53 +09:12:09.0 11.3mag 141P/Machholz
00:40:46.97 +00:49:01.7 11.4mag 141P-A/Machholz
23:31:58.06 -02:44:39.8 14.2mag 141P-D/Machholz
01:09:43.81 +02:27:49.2 17.9mag 141P-I/Machholz
00:32:16.04 -06:55:41.1 15.2mag 162P/SidingSpring
10:31:19.99 +31:33:55.7 17.8mag 164P/Christensen
06:16:32.37 +24:32:46.7 17.8mag 198P/ODAS
15:10:28.39 -01:19:38.5 17.3mag 210P/Christensen
21:05:32.84 -14:04:15.8 17.4mag 218P/LINEAR
17:11:59.76 -15:11:14.6 16.2mag 235P/LINEAR
05:11:30.54 +33:45:15.7 16.6mag 240P/NEAT
07:33:49.05 -06:24:44.8 17.6mag 242P/Spahr
15:46:12.96 +06:14:01.1 17.6mag 391P/Kowalski
07:30:38.15 +21:18:10.3 17.6mag 450P/LONEOS
05:20:29.44 +45:40:24.4 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 4 22:47 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 4 22:47 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
-rw-r--r-- 1 apache apache 187K Apr 4 22:47 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
13:12:45.220 +03:30:21.92 AT 2026hpi 2026-03-19.82 21.35
13:05:59.910 -01:19:19.75 AT 2026hph 2026-03-19.81 22.6
11:46:36.940 +01:57:40.33 AT 2026hpg 2026-03-19.65 22.05
11:30:33.790 +02:03:55.06 AT 2026hpf 2026-03-19.65 22.36
11:29:16.830 +01:43:15.67 AT 2026hpe 2026-03-19.65 22.04
11:20:49.830 +04:08:00.92 AT 2026hpd 2026-03-19.64 22
11:03:22.060 +00:37:39.12 AT 2026hpc 2026-03-19.63 22.18
10:52:11.360 -00:09:37.37 AT 2026hpb 2026-03-19.63 22.38
10:44:39.040 +03:59:23.53 AT 2026hpa 2026-03-19.63 22.2
10:39:27.590 +02:55:53.65 AT 2026hoz 2026-03-19.63 22.5
11:13:53.930 -02:04:37.04 AT 2026hoy 2026-03-19.57 22.08
11:32:56.040 +05:15:39.22 AT 2026hox 2026-03-13.75 21.79
14:19:03.910 +04:14:08.30 AT 2026how 2026-03-09.90 22.06
13:42:38.650 +04:05:57.15 AT 2026hov 2026-03-26.90 22.47
10:27:51.570 +00:48:59.98 AT 2026hou 2026-03-22.63 22.25
13:58:28.600 +02:11:38.08 AT 2026hot 2026-03-19.83 22.42
07:15:34.880 +25:58:24.77 AT 2026hos 2026-03-20.27 20.6179
06:14:25.910 +51:19:28.34 AT 2026hor 2026-03-25.14 20.2907
19:09:43.670 +04:40:04.90 AT 2026hoq 2026-03-25.91 16.32
13:14:45.263 +13:33:04.46 AT 2026hop 2026-03-28.45 19.632
-rw-r--r-- 1 apache apache 29K Apr 4 22:47 tns_transients_list.txt
