This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.89,0.05,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 20260417.1563 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.99,0.05,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 20260417.1563 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054040.72+415704.3,2461147.6563,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J054040.72+415704.3 20260417.1563 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.9379+44.9337,2461147.6563,13.45,0.05,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 J084.9379+44.9337 20260417.1563 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.9347+43.5066,2461147.6563,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.9347+43.5066 20260417.1563 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7193+43.4023,2461147.6563,13.29,0.05,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 J087.7193+43.4023 20260417.1563 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.7470+43.3200,2461147.6563,13.28,0.05,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 J089.7470+43.3200 20260417.1563 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196779978278037760,2461147.6563,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196779978278037760 20260417.1563 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.8907+42.6104,2461147.6563,13.29,0.05,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 J086.8907+42.6104 20260417.1563 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197434806172188416,2461147.6563,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197434806172188416 20260417.1563 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.2502+41.7761,2461147.6563,13.29,0.05,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 J086.2502+41.7761 20260417.1563 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 969934835279075072,2461147.6563,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 969934835279075072 20260417.1563 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.9297+43.1685,2461147.6563,13.26,0.05,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 J085.9297+43.1685 20260417.1563 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2781+45.3867,2461147.6563,13.03,0.05,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
ATO J089.2781+45.3867 20260417.1563 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197994904265884544,2461147.6563,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197994904265884544 20260417.1563 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J060214.12+474700.6,2461147.6563,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J060214.12+474700.6 20260417.1563 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J093.3290+41.8878,2461147.6563,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J093.3290+41.8878 20260417.1563 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.0519+42.7763,2461147.6563,12.85,0.05,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 J087.0519+42.7763 20260417.1563 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197875298016710784,2461147.6563,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197875298016710784 20260417.1563 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,12.88,0.05,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
target 20260417.1563 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192293833399060608,2461147.6563,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192293833399060608 20260417.1563 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.2531+46.4397,2461147.6563,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.2531+46.4397 20260417.1563 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.5437+43.6538,2461147.6563,12.61,0.05,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
ATO J087.5437+43.6538 20260417.1563 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J095.3673+41.8196,2461147.6563,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.3673+41.8196 20260417.1563 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 963145561432116096,2461147.6563,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 963145561432116096 20260417.1563 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196564783236506368,2461147.6563,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196564783236506368 20260417.1563 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196796848908972032,2461147.6563,12.41,0.05,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
Gaia DR3 196796848908972032 20260417.1563 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.4006+42.8245,2461147.6563,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J090.4006+42.8245 20260417.1563 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J054610.24+465447.5,2461147.6563,12.55,0.05,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
ASASSN-V J054610.24+465447.5 20260417.1563 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196601268981151360,2461147.6563,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 196601268981151360 20260417.1563 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J088.9474+42.5087,2461147.6563,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J088.9474+42.5087 20260417.1563 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211485843219678720,2461147.6563,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211485843219678720 20260417.1563 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.9948+43.8619,2461147.6563,12.84,0.05,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
ATO J089.9948+43.8619 20260417.1563 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.6351+48.1884,2461147.6563,12.84,0.05,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
ATO J090.6351+48.1884 20260417.1563 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197945941638987264,2461147.6563,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197945941638987264 20260417.1563 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1509+45.4814,2461147.6563,12.88,0.05,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
ATO J089.1509+45.4814 20260417.1563 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197388553666998656,2461147.6563,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197388553666998656 20260417.1563 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J084.3195+44.0466,2461147.6563,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J084.3195+44.0466 20260417.1563 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4626+44.3866,2461147.6563,13.05,0.05,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 J086.4626+44.3866 20260417.1563 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.02,0.05,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
target 20260417.1563 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.2776+47.3006,2461147.6563,13.19,0.05,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 J087.2776+47.3006 20260417.1563 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.09,0.05,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
target 20260417.1563 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.15,0.05,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 20260417.1563 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.1387+46.8868,2461147.6563,13.16,0.05,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
ATO J086.1387+46.8868 20260417.1563 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 192463089469495040,2461147.6563,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 192463089469495040 20260417.1563 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210216624548997760,2461147.6563,13.23,0.05,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 210216624548997760 20260417.1563 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J053745.20+455814.5,2461147.6563,13.26,0.05,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
ASASSN-V J053745.20+455814.5 20260417.1563 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 196552271996570368,2461147.6563,13.21,0.05,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 196552271996570368 20260417.1563 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.8054+43.8208,2461147.6563,13.29,0.05,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 J085.8054+43.8208 20260417.1563 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J090.2884+47.3636,2461147.6563,13.24,0.05,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 J090.2884+47.3636 20260417.1563 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J092.6873+48.2843,2461147.6563,13.18,0.05,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 J092.6873+48.2843 20260417.1563 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.38,0.05,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 20260417.1563 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197183292886359680,2461147.6563,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197183292886359680 20260417.1563 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 209612206687413376,2461147.6563,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 209612206687413376 20260417.1563 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210175117984104704,2461147.6563,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210175117984104704 20260417.1563 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.5381+48.6224,2461147.6563,13.38,0.05,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
ATO J089.5381+48.6224 20260417.1563 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 211249448220214656,2461147.6563,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 211249448220214656 20260417.1563 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J053518.21+473122.4,2461147.6563,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J053518.21+473122.4 20260417.1563 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J087.7475+43.1557,2461147.6563,13.64,0.05,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 J087.7475+43.1557 20260417.1563 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J086.4467+42.4827,2461147.6563,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J086.4467+42.4827 20260417.1563 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.88,0.05,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 20260417.1563 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1563 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J089.1705+47.6333,2461147.6563,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J089.1705+47.6333 20260417.1563 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6563,13.66,0.05,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 20260417.1563 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 210650661059367936,2461147.6563,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 210650661059367936 20260417.1563 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 197557981536079872,2461147.6563,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 197557981536079872 20260417.1563 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.5999+48.8035,2461147.6563,13.80,0.05,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 J085.5999+48.8035 20260417.1563 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J085.5013+48.1338,2461147.6563,13.89,0.05,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 J085.5013+48.1338 20260417.1563 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J096.8783+42.8003,2461147.6563,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.8783+42.8003 20260417.1563 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461147.65663762 17.04.2026 03:45:23.490 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16251
Objects passed selection criteria: 16215
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 13969.2
Average stars matched: 13614.8 (97.4623 %)
Memory usage VmPeak: 122836 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 22:53:41 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: 2461147.65663762 17.04.2026 03:45:23.490 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 261
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 91 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): 123167
Objects passed selection criteria: 122864
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: 109146
Average stars matched: 105407 (96.5743 %)
Memory usage VmPeak: 1960408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 22:56:44 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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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: 2461147.65600243
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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits'
wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits exists and is non-empty
Saving wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits to local_wcs_cache/
'wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 935.1'x631.3' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 05:59:47.823 +46:00:35.63 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:23.858 +46:00:47.94 J2000 4789.000 3195.000
###################################
###################################
# 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 06:00:23.858 +46:00:47.94
Angular distance between the image centers 0.1043 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:23.232 +46:00:20.30 J2000 4789.000 3195.000
###################################
###################################
# 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 06:00:23.232 +46:00:20.30
Angular distance between the image centers 0.1026 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 06:00:23.858 +46:00:47.94
Second-epoch second image center 06:00:23.232 +46:00:20.30
Angular distance between the image centers 0.00789 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.S5z3Ya0ifW
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.Y3F9IYQK3j
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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits &> /tmp/tmp.5VglXeIFas
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits &> /tmp/tmp.TidaGnkRZD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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 4 candidate transients before the final filtering. (Hard limit: 8000)
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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
2.7 pix fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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
14.8 mag. fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
14.8 mag. fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.8 (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.S5z3Ya0ifW (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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...
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...
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
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"
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.Y3F9IYQK3j (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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...
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...
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
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"
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.5VglXeIFas (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1029, passed=15652
Got 15652 stars (including 14614 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 15652 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 15390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 15391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 15391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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.TidaGnkRZD (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1049, passed=15597
Got 15597 stars (including 14538 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 15597 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 650 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...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 15310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 650 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
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 15309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 15309 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits'
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits'
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31045.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31045_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 31045_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:27:08.56 +45:54:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.662 965425669372973312 096.78623027583 +45.90568783677 12.1473 11.8113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31137_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 31137_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:14:58.98 +46:47:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31150_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 31150_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:59:43.42 +44:59:09.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31249_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 31249_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:42.90 +43:37:26.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field 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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits exists and is non-empty
wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits (1st reference image)
verification OK: wcs_Aur-02-Q2b1x1_2026-01-20_23-10-13_20.00sec_-14.90C_LIGHT_0227.fits
Image size: 935.1'x631.3' 15.6(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.86"/pix along the X axis and 5.93"/pix along the Y axis
Image center: 05:59:47.823 +46:00:35.63 J2000 4789.000 3195.000
###################################
The image scale is 5.86"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits (1st new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:23.858 +46:00:47.94 J2000 4789.000 3195.000
###################################
###################################
# 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 06:00:23.858 +46:00:47.94
Angular distance between the image centers 0.1043 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits (2nd new image)
verification OK: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
Image size: 937.5'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:00:23.232 +46:00:20.30 J2000 4789.000 3195.000
###################################
###################################
# 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 06:00:23.232 +46:00:20.30
Angular distance between the image centers 0.1026 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 06:00:23.858 +46:00:47.94
Second-epoch second image center 06:00:23.232 +46:00:20.30
Angular distance between the image centers 0.00789 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.QFTMGCyk1N
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.eUOE1cklYC
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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits &> /tmp/tmp.G2XvEhJtDa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits &> /tmp/tmp.Axj2MhCCiR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 215 candidate transients before the final filtering. (Hard limit: 8000)
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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
2.1 pix fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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
13.9 mag. fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
13.9 mag. fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QFTMGCyk1N (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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...
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...
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
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"
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.eUOE1cklYC (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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...
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...
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
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"
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.G2XvEhJtDa (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=10701, passed=115153
Got 115153 stars (including 104323 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 115153 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 650 to 708 (Dec 40.2 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...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 113566 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 650 to 708 (Dec 40.2 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
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 113567 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 113566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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.Axj2MhCCiR (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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=10504, passed=116024
Got 116024 stars (including 105398 good ones) from the SExtractor catalog wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 116024 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 650 to 708 (Dec 40.2 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...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 113595 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 650 to 708 (Dec 40.2 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
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 113592 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 113591 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits -region wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/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_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-44-28_20.00sec_-4.90C_LIGHT_0076.fits
Saving fully-calibrated image wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.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_2026-04-16_CI_Aur-02-Q2b1x1_224613_TTUQ2b1x1_3608185_ddtifKxw/wcs_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077.fits
Preparing the HTML report for the field Aur-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out192115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out194745.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out143438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192271.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193216.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__out193424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194754.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 115s
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: 45s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192112_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192112_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192115_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192115_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:47:59.92 +45:09:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.973 197600999930098944 086.99998403289 +45.16420702399 14.7507 13.8881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192118_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192118_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192125_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192125_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:50:10.21 +44:48:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.992 196782761416621824 087.54330890392 +44.81004374545 14.6933 14.2994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192132_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192132_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:15.26 +44:26:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.452 197155976895189888 084.81375248243 +44.44490986539 14.6048 13.9975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192134_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192134_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:59:30.19 +43:13:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.955 192523803127533056 089.87607557482 +43.22172424449 14.5691 14.0183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192143_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192143_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:58.32 +43:46:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.545 197043959850434688 084.74397659821 +43.77718805946 14.4957 13.8797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192144_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192144_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:50:37.06 +46:28:12.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192151_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192151_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192166_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192166_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:28.25 +46:16:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.367 209550187359249280 085.11742079075 +46.27087097741 14.4673 13.8137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192169_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192169_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192177_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192177_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:58:56.23 +42:40:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.798 192450337708214400 089.73443358118 +42.68352902876 14.0803 13.4942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192187_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192187_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192188_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192188_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:20.01 +41:55:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.637 193092800394897280 087.33390194821 +41.92263064796 14.2183 13.3818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192198_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192198_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192201_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192201_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:16.70 +42:10:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.477 192939040564836096 085.06976204516 +42.18288895315 14.4139 13.8388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192207_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192207_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192208_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192208_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192211_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192212_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192212_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:48:12.23 +42:34:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.111 192997516544670976 087.05160362420 +42.57714898017 13.9832 13.3947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192213_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192213_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192216_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192216_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:42:11.26 +44:17:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.590 197083787085250816 085.54707595404 +44.30000666857 14.3945 13.7235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192218_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192218_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192222_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192222_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192229_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192229_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:24:04.04 +44:40:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.152 959256898041674880 096.01653084857 +44.67501473517 13.9280 13.3588 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192230_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192230_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192235_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192235_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192239_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192239_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:47:50.26 +43:23:25.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192241_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192241_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192242_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192242_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:46.48 +47:09:33.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192243_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192243_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:41:26.73 +43:07:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192248_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192248_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192252_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192252_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:40.46 +44:00:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192256_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192256_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:27:52.63 +42:46:55.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192263_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192263_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:29.52 +46:12:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.488 209537817853642752 085.12292055667 +46.20279066372 14.1709 13.3563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192264_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192264_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192271_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192271_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192276_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192276_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:44:36.78 +46:43:35.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192278_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192278_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:47:48.85 +43:07:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192279_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192279_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:50:32.91 +42:15:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192285_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192285_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192286_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192286_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192288_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192288_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:19.11 +41:34:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.741 191385087037913344 084.57987545906 +41.57149786600 13.4742 12.6431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192293_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192293_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:46:16.90 +43:28:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192294_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192294_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:05:26.88 +42:40:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192301_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192301_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:43:57.10 +41:54:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.732 192765386447163008 085.98811596338 +41.90076320551 13.8104 13.0397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192305_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192305_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192308_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192308_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192309_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192309_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192310_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192310_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:25.07 +48:02:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192313_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192313_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192314_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192314_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192315_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192315_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192320_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192320_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:53.93 +47:59:43.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192321_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192321_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:56:29.59 +45:53:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.752 196978848146463360 089.12358565363 +45.88965312854 13.5594 12.7709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192325_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192325_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192327_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192327_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192334_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192334_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:16:36.30 +44:32:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.572 962371397869379840 094.15117384056 +44.54909987079 13.3865 12.9906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192335_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192335_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:25:09.25 +42:30:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 2.088 958643507992958208 096.28799370544 +42.51269412246 13.0165 12.4700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192339_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192339_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:31:07.02 +48:10:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192345_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192345_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:36:47.05 +42:57:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192346_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192346_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:29:14.82 +41:54:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192349_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192349_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:42:01.66 +46:28:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192350_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192350_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:34.95 +43:13:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.914 193447530333092992 087.39597223618 +43.22632607761 13.2284 12.4372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192351_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192351_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:11:13.04 +47:02:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192353_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192353_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:43:17.27 +42:28:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192357_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192357_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192358_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192358_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:20:13.24 +43:38:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 0.580 961773886316261504 095.05528574915 +43.64410819835 12.5992 12.1017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192362_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192362_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:23.51 +49:53:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192364_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192364_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:23.69 +44:31:31.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192365_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192365_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:55.27 +42:54:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 0.436 196195961507760768 084.48025002876 +42.90529955301 12.0708 11.0475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192366_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192366_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:45.99 +43:34:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192367_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192367_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:08.90 +46:13:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192372_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192372_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:43:27.56 +42:19:24.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192474_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192474_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:28.49 +43:00:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192504_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192504_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:22.95 +46:49:18.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192594_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192594_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:42.89 +43:37:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192674_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192674_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:11:34.47 +48:44:35.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192701_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192701_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:19.53 +42:40:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192765_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192765_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:01.41 +42:24:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 0.393 194493264674184192 084.25595370453 +42.40004651551 12.4117 11.9178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192766_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192766_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:46:26.48 +47:55:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192859_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192859_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:17.67 +45:03:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192878_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192878_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:48:04.11 +43:19:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192885_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192885_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:19:04.16 +47:21:53.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192900_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 192900_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192975_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192975_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:02.79 +50:02:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192978_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 192978_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:07.56 +44:53:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193041_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193041_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:03.11 +42:12:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193063_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193063_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:05:50.16 +44:39:31.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193066_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193066_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:48:45.95 +46:35:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193113_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193113_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:23.83 +47:29:29.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193133_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193133_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:43.09 +48:20:09.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193185_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193185_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193188_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193188_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:47:16.12 +46:04:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193192_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193192_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:46.05 +45:53:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193211_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193211_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:02.38 +49:49:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193216_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193216_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193224_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193224_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:14.20 +50:00:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193234_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193234_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:03:13.63 +42:56:26.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193266_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193266_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:47:45.29 +50:03:05.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193281_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193281_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193282_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193282_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193296_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193296_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:25.87 +48:47:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193327_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193327_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:44.78 +44:40:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.545 196778530872462720 087.43708391040 +44.68054544005 13.3227 12.4168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193333_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193333_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:46.28 +43:03:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193382_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193382_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:01:04.61 +50:00:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193400_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193400_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:17:34.63 +46:23:45.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193411_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193411_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:52:03.67 +49:32:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193424_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193424_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193445_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193445_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193462_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193462_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:46.39 +46:04:00.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193465_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193465_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193492_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193492_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193546_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193546_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:28.20 +42:14:30.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193553_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193553_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:32.66 +41:57:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193564_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193564_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:22.06 +42:59:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193599_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193599_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193607_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193607_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193615_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193615_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:35:35.25 +44:15:15.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193622_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193622_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:00:13.98 +47:43:14.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193624_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193624_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:43:56.68 +47:43:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.182 209945083832417792 085.98700751845 +47.73238449856 13.7368 12.8375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193629_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193629_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193650_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193650_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:52:21.12 +42:50:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193653_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193653_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:18.71 +47:12:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.612 210617675710733440 084.07861717601 +47.20262819261 13.8371 13.0109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193663_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193663_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:44:39.71 +43:57:56.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193667_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193667_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193668_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193668_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:53:31.09 +44:15:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 1.152 196520424814484992 088.37994109512 +44.25250419597 13.6666 13.0703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193674_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193674_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:50.41 +49:49:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193687_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193687_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:18.56 +44:01:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193716_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193716_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193722_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193722_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:49.69 +45:56:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.470 209517442528660352 084.45762274013 +45.93852533875 14.0344 13.4496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193726_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193726_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:30.28 +43:50:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.131 195602744923203072 084.12617236068 +43.84724153440 13.5985 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193728_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193728_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:27.88 +47:51:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.212 210289162252676480 087.36624514415 +47.85569300332 13.8992 13.3131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193746_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193746_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:06.30 +45:12:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193755_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193755_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193774_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193774_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:01:16.74 +47:35:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193775_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193775_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193776_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193776_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:46:39.70 +43:21:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.284 196091031163933312 086.66581728830 +43.35265011844 13.5868 12.7257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193789_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193789_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193794_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193794_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:42:50.75 +48:07:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.557 210768240084034432 085.71251702241 +48.12734957677 13.8686 13.1085 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193818_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193818_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:48:44.67 +49:34:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.976 211467323320736640 087.18633608971 +49.57803964372 13.8597 13.0929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193821_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193821_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193827_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193827_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193828_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193828_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193829_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193829_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:32.18 +47:15:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.912 210597025508196480 084.63478085416 +47.26331477231 14.1422 13.2923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193832_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193832_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:24.29 +42:59:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193839_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193839_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193880_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193880_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:42:16.11 +43:16:24.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193885_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193885_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:35:41.31 +44:16:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193898_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193898_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:25:45.38 +45:22:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193921_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193921_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:57.46 +42:25:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193931_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193931_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:24.76 +49:14:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.112 210526725482759552 089.35356580650 +49.24269354636 13.7503 12.9166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193937_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193937_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:44.68 +42:36:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.526 195999702979561088 084.43666045147 +42.61096798820 14.0108 13.3796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193953_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193953_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193965_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193965_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193979_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 193979_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193986_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 193986_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:24.68 +43:50:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194002_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194002_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194005_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194005_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:17:15.33 +42:06:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194007_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194007_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:55.45 +45:00:39.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194020_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194020_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:07.25 +47:47:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.004 210851425010949248 084.03053518535 +47.79032813681 14.0727 13.2386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194045_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194045_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194054_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194054_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:12:19.96 +50:12:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194093_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194093_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:23.35 +49:49:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.500 214254619657430144 084.84769115489 +49.82477197399 14.0502 13.3596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194101_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194101_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:53:58.74 +46:09:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194111_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194111_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194118_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194118_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194121_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194121_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:59.80 +47:35:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.406 210652963161786496 084.74933016926 +47.59227422075 14.1786 13.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194122_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194122_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194189_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194189_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194205_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194205_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:03:02.73 +46:43:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194225_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194225_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194240_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194240_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194277_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194277_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194285_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194285_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:41:07.31 +47:58:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194298_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194298_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:13.55 +44:55:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.129 196664632636062336 089.30690131675 +44.92317349648 14.3868 13.6231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194304_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194304_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194327_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194327_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194375_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194375_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194387_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194387_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194422_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194422_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194472_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194472_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194474_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194474_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:54:16.06 +41:58:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.149 192299846352802176 088.56714256474 +41.96732700967 14.4620 13.6806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194507_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194507_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194529_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194529_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194543_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194543_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194549_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194549_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194560_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194560_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:18.59 +45:28:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 0.522 196927450274785792 089.32765314131 +45.48035392189 14.4964 13.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194598_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194598_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194610_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194610_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:43.93 +46:33:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.471 209742773692634624 084.93363579767 +46.55265746365 14.7565 14.0907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194613_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194613_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:27.60 +44:12:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.600 197091140068942208 084.86518804408 +44.21392982565 14.5965 13.7480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194628_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194628_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:35:48.81 +47:50:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.233 210849603944817664 083.95385514517 +47.83981062777 14.4444 13.5806 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194630_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194630_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:34.35 +42:20:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.399 195935209751002752 084.89360411427 +42.33684241881 14.4030 13.4477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194639_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194639_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194644_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194644_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194679_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194679_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194683_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194683_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194695_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194695_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194696_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194696_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:11.97 +46:08:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.337 209542422058414464 084.80022765244 +46.14755365067 14.6189 13.7869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194705_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194705_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:13.15 +46:56:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.260 210554247633988736 084.30529867553 +46.94214321817 14.9291 14.2628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194712_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194712_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194720_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194720_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:40:09.10 +43:18:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.406 196241664257129856 085.03844580851 +43.30109303773 14.5371 13.7195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194727_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194727_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:44:04.87 +42:22:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 0.898 193024218356310912 086.02059551907 +42.37752556588 14.8086 14.0508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194744_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194744_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:53:33.73 +45:10:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.190 196815231368805120 088.39086657124 +45.17129384205 14.8476 14.1717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194745_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194745_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:30.43 +44:27:02.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194752_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194752_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194754_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 194754_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194769_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194769_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:06.78 +46:01:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.738 209529193559420160 084.77854411303 +46.01887038938 14.7570 14.0286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194772_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194772_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:18.69 +46:40:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.828 209759575604369920 084.82861277952 +46.67351168016 14.8166 14.1638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194788_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 194788_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:30.74 +45:46:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.411 197511119150017024 086.37854119210 +45.77189386909 14.7959 14.0459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143438_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
Preparing report for the candidate 143438_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41230_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 41230_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:57:24.01 +48:22:39.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52500_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 52500_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:59:44.12 +47:37:00.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102378_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 102378_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 05:37:57.05 +44:41:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63136_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077
The candidate 63136_fd_Aur-02-Q2b1x1_2026-04-16_22-45-23_20.00sec_-4.90C_LIGHT_0077 did not pass the final checks
**** FOUND 06:14:58.94 +46:47:46.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 165s
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 ####
06:27:32.31 +42:47:54.6
06:04:37.00 +48:46:00.1
05:51:13.67 +47:13:42.0
05:55:07.54 +43:53:52.0
05:40:40.75 +41:57:02.5
05:39:45.69 +44:56:09.1
05:47:44.75 +43:30:51.4
05:50:53.13 +43:23:59.2
05:58:56.70 +43:19:44.6
05:50:24.30 +44:44:49.9
05:47:29.48 +42:36:36.8
05:41:02.66 +45:28:13.6
05:44:58.36 +41:46:34.1
06:27:28.53 +41:47:01.7
06:02:17.93 +49:12:45.1
05:43:43.06 +43:10:05.0
05:57:08.95 +45:23:02.7
05:52:59.16 +46:57:29.5
06:24:58.07 +42:35:44.3
06:02:14.44 +47:47:01.6
06:13:19.17 +41:52:41.3
05:48:13.25 +42:46:41.8
05:59:43.72 +47:14:06.4
06:08:44.08 +48:20:44.3
05:54:08.29 +41:46:21.4
05:56:59.24 +46:26:55.8
05:50:10.20 +43:38:47.9
06:21:31.83 +41:49:28.4
06:01:39.47 +45:44:14.7
05:49:28.95 +44:16:19.2
05:53:06.81 +44:56:00.2
06:12:10.20 +50:14:53.6
06:01:31.74 +42:49:22.1
05:46:10.02 +46:54:48.1
05:52:15.63 +44:44:13.2
05:55:48.03 +42:30:31.8
05:48:23.14 +49:46:57.8
05:59:59.06 +43:51:29.3
06:02:32.02 +48:11:24.2
05:51:18.84 +43:17:45.9
05:57:11.96 +42:33:34.2
05:53:28.88 +46:52:04.5
05:56:33.83 +45:29:09.6
05:37:19.25 +44:51:38.8
06:03:21.19 +42:41:50.6
05:37:16.42 +44:02:46.6
05:39:19.10 +44:01:55.5
05:45:50.34 +44:23:04.2
05:57:11.33 +42:50:25.4
05:49:06.45 +47:17:57.9
05:56:28.33 +47:43:41.1
05:49:38.57 +47:49:50.3
05:44:33.88 +46:53:12.8
05:54:37.56 +42:21:15.8
05:55:10.37 +48:15:53.0
05:37:41.35 +45:58:10.0
05:50:28.77 +44:11:35.0
05:43:13.13 +43:49:15.1
06:01:02.32 +47:22:14.6
06:10:45.04 +48:16:54.8
05:53:49.40 +48:01:12.0
06:01:43.62 +48:26:05.5
05:43:59.69 +44:30:07.3
05:44:47.03 +46:28:21.9
05:57:11.23 +48:02:14.6
05:58:09.50 +48:37:12.3
05:49:29.22 +42:28:09.4
05:54:17.72 +49:03:41.7
05:35:18.16 +47:31:20.2
05:52:19.78 +47:40:07.7
05:51:01.96 +43:08:51.3
05:45:48.59 +42:29:30.2
05:51:34.79 +49:56:50.0
05:37:40.67 +42:09:38.9
05:56:39.20 +47:38:09.4
06:00:47.24 +44:57:02.3
05:38:34.95 +47:30:21.8
05:43:48.37 +46:02:53.4
05:42:24.49 +48:48:10.7
05:41:57.60 +48:08:20.0
########### 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 ####
06:04:37.00 +48:46:00.1
05:51:13.67 +47:13:42.0
05:55:07.54 +43:53:52.0
05:40:40.75 +41:57:02.5
05:39:45.69 +44:56:09.1
05:47:44.75 +43:30:51.4
05:50:53.13 +43:23:59.2
05:58:56.70 +43:19:44.6
05:50:24.30 +44:44:49.9
05:47:29.48 +42:36:36.8
05:41:02.66 +45:28:13.6
05:44:58.36 +41:46:34.1
06:27:28.53 +41:47:01.7
06:02:17.93 +49:12:45.1
05:43:43.06 +43:10:05.0
05:57:08.95 +45:23:02.7
05:52:59.16 +46:57:29.5
06:24:58.07 +42:35:44.3
06:02:14.44 +47:47:01.6
06:13:19.17 +41:52:41.3
05:48:13.25 +42:46:41.8
05:59:43.72 +47:14:06.4
06:08:44.08 +48:20:44.3
05:54:08.29 +41:46:21.4
05:56:59.24 +46:26:55.8
05:50:10.20 +43:38:47.9
06:21:31.83 +41:49:28.4
06:01:39.47 +45:44:14.7
05:49:28.95 +44:16:19.2
05:53:06.81 +44:56:00.2
06:12:10.20 +50:14:53.6
06:01:31.74 +42:49:22.1
05:46:10.02 +46:54:48.1
05:52:15.63 +44:44:13.2
05:55:48.03 +42:30:31.8
05:48:23.14 +49:46:57.8
05:59:59.06 +43:51:29.3
06:02:32.02 +48:11:24.2
05:51:18.84 +43:17:45.9
05:57:11.96 +42:33:34.2
05:53:28.88 +46:52:04.5
05:56:33.83 +45:29:09.6
05:37:19.25 +44:51:38.8
06:03:21.19 +42:41:50.6
05:37:16.42 +44:02:46.6
05:39:19.10 +44:01:55.5
05:45:50.34 +44:23:04.2
05:57:11.33 +42:50:25.4
05:49:06.45 +47:17:57.9
05:56:28.33 +47:43:41.1
05:49:38.57 +47:49:50.3
05:44:33.88 +46:53:12.8
05:54:37.56 +42:21:15.8
05:55:10.37 +48:15:53.0
05:37:41.35 +45:58:10.0
05:50:28.77 +44:11:35.0
05:43:13.13 +43:49:15.1
06:01:02.32 +47:22:14.6
06:10:45.04 +48:16:54.8
05:53:49.40 +48:01:12.0
06:01:43.62 +48:26:05.5
05:43:59.69 +44:30:07.3
05:44:47.03 +46:28:21.9
05:57:11.23 +48:02:14.6
05:58:09.50 +48:37:12.3
05:49:29.22 +42:28:09.4
05:54:17.72 +49:03:41.7
05:35:18.16 +47:31:20.2
05:52:19.78 +47:40:07.7
05:51:01.96 +43:08:51.3
05:45:48.59 +42:29:30.2
05:51:34.79 +49:56:50.0
05:37:40.67 +42:09:38.9
05:56:39.20 +47:38:09.4
06:00:47.24 +44:57:02.3
05:38:34.95 +47:30:21.8
05:43:48.37 +46:02:53.4
05:42:24.49 +48:48:10.7
05:41:57.60 +48:08:20.0
06:27:32.31 +42:47:54.6
###################################################################################
06:04:37.00 +48:46:00.1 -- not an asteroid (will add it to exclusion list)
05:51:13.67 +47:13:42.0 -- not an asteroid (will add it to exclusion list)
05:55:07.54 +43:53:52.0 -- not an asteroid (will add it to exclusion list)
05:40:40.75 +41:57:02.5 -- not an asteroid (will add it to exclusion list)
05:39:45.69 +44:56:09.1 -- not an asteroid (will add it to exclusion list)
05:47:44.75 +43:30:51.4 -- not an asteroid (will add it to exclusion list)
05:50:53.13 +43:23:59.2 -- not an asteroid (will add it to exclusion list)
05:58:56.70 +43:19:44.6 -- not an asteroid (will add it to exclusion list)
05:50:24.30 +44:44:49.9 -- not an asteroid (will add it to exclusion list)
05:47:29.48 +42:36:36.8 -- not an asteroid (will add it to exclusion list)
05:41:02.66 +45:28:13.6 -- not an asteroid (will add it to exclusion list)
05:44:58.36 +41:46:34.1 -- not an asteroid (will add it to exclusion list)
06:27:28.53 +41:47:01.7 -- not an asteroid (will add it to exclusion list)
06:02:17.93 +49:12:45.1 -- not an asteroid (will add it to exclusion list)
05:43:43.06 +43:10:05.0 -- not an asteroid (will add it to exclusion list)
05:57:08.95 +45:23:02.7 -- not an asteroid (will add it to exclusion list)
05:52:59.16 +46:57:29.5 -- not an asteroid (will add it to exclusion list)
06:24:58.07 +42:35:44.3 -- not an asteroid (will add it to exclusion list)
06:02:14.44 +47:47:01.6 -- not an asteroid (will add it to exclusion list)
06:13:19.17 +41:52:41.3 -- not an asteroid (will add it to exclusion list)
05:48:13.25 +42:46:41.8 -- not an asteroid (will add it to exclusion list)
05:59:43.72 +47:14:06.4 -- not an asteroid (will add it to exclusion list)
06:08:44.08 +48:20:44.3 -- not an asteroid (will add it to exclusion list)
05:54:08.29 +41:46:21.4 -- not an asteroid (will add it to exclusion list)
05:56:59.24 +46:26:55.8 -- not an asteroid (will add it to exclusion list)
05:50:10.20 +43:38:47.9 -- not an asteroid (will add it to exclusion list)
06:21:31.83 +41:49:28.4 -- not an asteroid (will add it to exclusion list)
06:01:39.47 +45:44:14.7 -- not an asteroid (will add it to exclusion list)
05:49:28.95 +44:16:19.2 -- not an asteroid (will add it to exclusion list)
05:53:06.81 +44:56:00.2 -- not an asteroid (will add it to exclusion list)
06:12:10.20 +50:14:53.6 -- not an asteroid (will add it to exclusion list)
06:01:31.74 +42:49:22.1 -- not an asteroid (will add it to exclusion list)
05:46:10.02 +46:54:48.1 -- not an asteroid (will add it to exclusion list)
05:52:15.63 +44:44:13.2 -- not an asteroid (will add it to exclusion list)
05:55:48.03 +42:30:31.8 -- not an asteroid (will add it to exclusion list)
05:48:23.14 +49:46:57.8 -- not an asteroid (will add it to exclusion list)
05:59:59.06 +43:51:29.3 -- not an asteroid (will add it to exclusion list)
06:02:32.02 +48:11:24.2 -- not an asteroid (will add it to exclusion list)
05:51:18.84 +43:17:45.9 -- not an asteroid (will add it to exclusion list)
05:57:11.96 +42:33:34.2 -- not an asteroid (will add it to exclusion list)
05:53:28.88 +46:52:04.5 -- not an asteroid (will add it to exclusion list)
05:56:33.83 +45:29:09.6 -- not an asteroid (will add it to exclusion list)
05:37:19.25 +44:51:38.8 -- not an asteroid (will add it to exclusion list)
06:03:21.19 +42:41:50.6 -- not an asteroid (will add it to exclusion list)
05:37:16.42 +44:02:46.6 -- not an asteroid (will add it to exclusion list)
05:39:19.10 +44:01:55.5 -- not an asteroid (will add it to exclusion list)
05:45:50.34 +44:23:04.2 -- not an asteroid (will add it to exclusion list)
05:57:11.33 +42:50:25.4 -- not an asteroid (will add it to exclusion list)
05:49:06.45 +47:17:57.9 -- not an asteroid (will add it to exclusion list)
05:56:28.33 +47:43:41.1 -- not an asteroid (will add it to exclusion list)
05:49:38.57 +47:49:50.3 -- not an asteroid (will add it to exclusion list)
05:44:33.88 +46:53:12.8 -- not an asteroid (will add it to exclusion list)
05:54:37.56 +42:21:15.8 -- not an asteroid (will add it to exclusion list)
05:55:10.37 +48:15:53.0 -- not an asteroid (will add it to exclusion list)
05:37:41.35 +45:58:10.0 -- not an asteroid (will add it to exclusion list)
05:50:28.77 +44:11:35.0 -- not an asteroid (will add it to exclusion list)
05:43:13.13 +43:49:15.1 -- not an asteroid (will add it to exclusion list)
06:01:02.32 +47:22:14.6 -- not an asteroid (will add it to exclusion list)
06:10:45.04 +48:16:54.8 -- not an asteroid (will add it to exclusion list)
05:53:49.40 +48:01:12.0 -- not an asteroid (will add it to exclusion list)
06:01:43.62 +48:26:05.5 -- not an asteroid (will add it to exclusion list)
05:43:59.69 +44:30:07.3 -- not an asteroid (will add it to exclusion list)
05:44:47.03 +46:28:21.9 -- not an asteroid (will add it to exclusion list)
05:57:11.23 +48:02:14.6 -- not an asteroid (will add it to exclusion list)
05:58:09.50 +48:37:12.3 -- not an asteroid (will add it to exclusion list)
05:49:29.22 +42:28:09.4 -- not an asteroid (will add it to exclusion list)
05:54:17.72 +49:03:41.7 -- not an asteroid (will add it to exclusion list)
05:35:18.16 +47:31:20.2 -- not an asteroid (will add it to exclusion list)
05:52:19.78 +47:40:07.7 -- not an asteroid (will add it to exclusion list)
05:51:01.96 +43:08:51.3 -- not an asteroid (will add it to exclusion list)
05:45:48.59 +42:29:30.2 -- not an asteroid (will add it to exclusion list)
05:51:34.79 +49:56:50.0 -- not an asteroid (will add it to exclusion list)
05:37:40.67 +42:09:38.9 -- not an asteroid (will add it to exclusion list)
05:56:39.20 +47:38:09.4 -- not an asteroid (will add it to exclusion list)
06:00:47.24 +44:57:02.3 -- not an asteroid (will add it to exclusion list)
05:38:34.95 +47:30:21.8 -- not an asteroid (will add it to exclusion list)
05:43:48.37 +46:02:53.4 -- not an asteroid (will add it to exclusion list)
05:42:24.49 +48:48:10.7 -- not an asteroid (will add it to exclusion list)
05:41:57.60 +48:08:20.0 -- not an asteroid (will add it to exclusion list)
06:27:32.31 +42:47:54.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
05:35:18.16 +47:31:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:16.42 +44:02:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:19.25 +44:51:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:40.67 +42:09:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:41.35 +45:58:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:34.95 +47:30:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:19.10 +44:01:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:45.69 +44:56:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:40.75 +41:57:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:02.66 +45:28:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:57.60 +48:08:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:24.49 +48:48:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:13.13 +43:49:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:43.06 +43:10:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:48.37 +46:02:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:59.69 +44:30:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:33.88 +46:53:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:47.03 +46:28:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:58.36 +41:46:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:48.59 +42:29:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:50.34 +44:23:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:10.02 +46:54:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:29.48 +42:36:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:44.75 +43:30:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:13.25 +42:46:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:23.14 +49:46:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:06.45 +47:17:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:28.95 +44:16:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:29.22 +42:28:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:38.57 +47:49:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:10.20 +43:38:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:24.30 +44:44:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:28.77 +44:11:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:53.13 +43:23:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:01.96 +43:08:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:13.67 +47:13:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:18.84 +43:17:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:34.79 +49:56:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:15.63 +44:44:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:19.78 +47:40:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:59.16 +46:57:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:06.81 +44:56:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:28.88 +46:52:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:49.40 +48:01:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:08.29 +41:46:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:17.72 +49:03:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:37.56 +42:21:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:07.54 +43:53:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:10.37 +48:15:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:48.03 +42:30:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:28.33 +47:43:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:33.83 +45:29:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:39.20 +47:38:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:59.24 +46:26:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:08.95 +45:23:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.23 +48:02:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.33 +42:50:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:11.96 +42:33:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:09.50 +48:37:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:56.70 +43:19:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:43.72 +47:14:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:59.06 +43:51:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:00:47.24 +44:57:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:02.32 +47:22:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:31.74 +42:49:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:39.47 +45:44:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:43.62 +48:26:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:14.44 +47:47:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:17.93 +49:12:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:32.02 +48:11:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:21.19 +42:41:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:04:37.00 +48:46:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:44.08 +48:20:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:45.04 +48:16:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:10.20 +50:14:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:13:19.17 +41:52:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:21:31.83 +41:49:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:58.07 +42:35:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:28.53 +41:47:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:32.31 +42:47:54.6 -- 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)
05:35:18.16 +47:31:20.2 -- a known variable star
05:37:16.42 +44:02:46.6 -- not a known variable star
05:37:19.25 +44:51:38.8 -- not a known variable star
05:37:40.67 +42:09:38.9 -- not a known variable star
05:37:41.35 +45:58:10.0 -- not a known variable star
05:38:34.95 +47:30:21.8 -- a known variable star
05:39:19.10 +44:01:55.5 -- not a known variable star
05:39:45.69 +44:56:09.1 -- not a known variable star
05:40:40.75 +41:57:02.5 -- a known variable star
05:41:02.66 +45:28:13.6 -- a known variable star
05:41:57.60 +48:08:20.0 -- not a known variable star
05:42:24.49 +48:48:10.7 -- not a known variable star
05:43:13.13 +43:49:15.1 -- not a known variable star
05:43:43.06 +43:10:05.0 -- not a known variable star
05:43:48.37 +46:02:53.4 -- not a known variable star
05:43:59.69 +44:30:07.3 -- a known variable star
05:44:33.88 +46:53:12.8 -- not a known variable star
05:44:47.03 +46:28:21.9 -- not a known variable star
05:44:58.36 +41:46:34.1 -- not a known variable star
05:45:48.59 +42:29:30.2 -- not a known variable star
05:45:50.34 +44:23:04.2 -- not a known variable star
05:46:10.02 +46:54:48.1 -- a known variable star
05:47:29.48 +42:36:36.8 -- not a known variable star
05:47:44.75 +43:30:51.4 -- not a known variable star
05:48:13.25 +42:46:41.8 -- not a known variable star
05:48:23.14 +49:46:57.8 -- not a known variable star
05:49:06.45 +47:17:57.9 -- not a known variable star
05:49:28.95 +44:16:19.2 -- not a known variable star
05:49:29.22 +42:28:09.4 -- not a known variable star
05:49:38.57 +47:49:50.3 -- not a known variable star
05:50:10.20 +43:38:47.9 -- not a known variable star
05:50:24.30 +44:44:49.9 -- not a known variable star
05:50:28.77 +44:11:35.0 -- a known variable star
05:50:53.13 +43:23:59.2 -- not a known variable star
05:51:01.96 +43:08:51.3 -- not a known variable star
05:51:13.67 +47:13:42.0 -- not a known variable star
05:51:18.84 +43:17:45.9 -- not a known variable star
05:51:34.79 +49:56:50.0 -- not a known variable star
05:52:15.63 +44:44:13.2 -- not a known variable star
05:52:19.78 +47:40:07.7 -- not a known variable star
05:52:59.16 +46:57:29.5 -- not a known variable star
05:53:06.81 +44:56:00.2 -- not a known variable star
05:53:28.88 +46:52:04.5 -- not a known variable star
05:53:49.40 +48:01:12.0 -- not a known variable star
05:54:08.29 +41:46:21.4 -- a known variable star
05:54:17.72 +49:03:41.7 -- not a known variable star
05:54:37.56 +42:21:15.8 -- a known variable star
05:55:07.54 +43:53:52.0 -- not a known variable star
05:55:10.37 +48:15:53.0 -- not a known variable star
05:55:48.03 +42:30:31.8 -- not a known variable star
05:56:28.33 +47:43:41.1 -- not a known variable star
05:56:33.83 +45:29:09.6 -- not a known variable star
05:56:39.20 +47:38:09.4 -- not a known variable star
05:56:59.24 +46:26:55.8 -- not a known variable star
05:57:08.95 +45:23:02.7 -- not a known variable star
05:57:11.23 +48:02:14.6 -- not a known variable star
05:57:11.33 +42:50:25.4 -- not a known variable star
05:57:11.96 +42:33:34.2 -- not a known variable star
05:58:09.50 +48:37:12.3 -- not a known variable star
05:58:56.70 +43:19:44.6 -- not a known variable star
05:59:43.72 +47:14:06.4 -- not a known variable star
05:59:59.06 +43:51:29.3 -- not a known variable star
06:00:47.24 +44:57:02.3 -- not a known variable star
06:01:02.32 +47:22:14.6 -- not a known variable star
06:01:31.74 +42:49:22.1 -- not a known variable star
06:01:39.47 +45:44:14.7 -- not a known variable star
06:01:43.62 +48:26:05.5 -- not a known variable star
06:02:14.44 +47:47:01.6 -- a known variable star
06:02:17.93 +49:12:45.1 -- not a known variable star
06:02:32.02 +48:11:24.2 -- not a known variable star
06:03:21.19 +42:41:50.6 -- not a known variable star
06:04:37.00 +48:46:00.1 -- not a known variable star
06:08:44.08 +48:20:44.3 -- not a known variable star
06:10:45.04 +48:16:54.8 -- not a known variable star
06:12:10.20 +50:14:53.6 -- not a known variable star
06:13:19.17 +41:52:41.3 -- not a known variable star
06:21:31.83 +41:49:28.4 -- not a known variable star
06:24:58.07 +42:35:44.3 -- not a known variable star
06:27:28.53 +41:47:01.7 -- not a known variable star
06:27:32.31 +42:47:54.6 -- not a known variable star
Found 70 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
80 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 80 (excluding asteroids and hot pixels, 70 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)2461147.65600243 -observatory V36
00:13:27.40 -01:24:32.1 Mercury (0.0mag)
03:14:18.60 +18:17:08.8 Venus (-3.9mag)
00:21:07.39 +01:13:32.6 Mars (1.2mag)
07:13:09.77 +22:45:21.3 Jupiter (-2.1mag)
00:29:41.71 +00:52:10.9 Saturn (0.9mag)
03:47:56.49 +19:48:15.6 Uranus (5.8mag)
00:10:59.45 -00:14:25.4 Neptune (7.8mag)
20:33:48.22 -22:52:39.3 Pluto (14.5mag)
01:14:09.55 +11:18:20.0 Moon (99.9mag)
-rw-r--r-- 1 apache apache 361 Apr 16 22:53 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461147.65600243:
07:13:04.96 +22:45:29.1 Io (5.8mag)
07:13:19.70 +22:44:58.0 Europa (5.9mag)
07:13:11.91 +22:45:09.5 Ganymede (5.4mag)
07:13:42.72 +22:44:09.9 Callisto (6.6mag)
07:16:26.92 +22:32:26.9 Himalia (15.3mag)
07:13:12.99 +22:45:15.6 Thebe (16.2mag)
07:16:39.76 +23:02:42.7 Elara (17.3mag)
07:12:07.38 +23:24:45.3 Pasiphae (17.4mag)
07:21:27.91 +22:43:29.2 Carme (18.5mag)
00:29:38.14 +00:52:38.8 Titan (8.8mag)
00:29:46.29 +00:52:09.9 Rhea (10.1mag)
00:29:19.83 +00:52:09.2 Iapetus (11.5mag)
00:29:45.72 +00:52:35.7 Hyperion (14.8mag)
00:31:17.68 +01:00:51.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 16 22:53 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461147.65600243:
15:43:28.84 -17:03:02.3 JWST
17:40:42.88 +38:25:33.0 Chandra
17:18:28.45 -47:58:37.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 16 22:53 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461147.65600243 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:27.52 -28:50:50.5 13.9mag P/2010 H2 (Vales)
05:07:34.33 -69:36:27.6 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:42.02 +31:26:43.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:18.81 +10:41:02.4 17.6mag C/2021 G2 (ATLAS)
23:10:31.52 +29:16:30.8 17.1mag C/2022 E2 (ATLAS)
04:30:35.18 +26:04:10.5 16.0mag C/2022 N2 (PANSTARRS)
09:03:40.79 +32:01:24.6 16.2mag C/2022 QE78 (ATLAS)
08:31:15.56 -00:01:54.4 17.3mag C/2022 R6 (PANSTARRS)
18:53:26.84 +18:37:44.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:40:17.65 -11:30:16.6 17.5mag P/2023 B1 (PANSTARRS)
09:07:06.87 -11:41:57.6 17.6mag C/2023 F3 (ATLAS)
21:55:21.36 +62:58:29.4 17.5mag C/2023 H5 (Lemmon)
19:18:10.34 -03:45:09.0 14.1mag C/2023 R1 (PANSTARRS)
21:29:57.60 +86:04:20.8 17.8mag C/2023 X2 (Lemmon)
06:18:27.55 +63:30:30.7 17.2mag C/2024 A1 (ATLAS)
05:15:44.09 +18:41:04.0 11.1mag C/2024 E1 (Wierzchos)
16:18:31.44 +06:34:46.6 17.4mag C/2024 G6 (ATLAS)
20:21:07.42 +15:35:23.3 14.6mag C/2024 J3 (ATLAS)
03:27:24.63 -22:12:38.2 16.3mag C/2024 T5 (ATLAS)
05:17:41.90 +45:00:23.3 17.7mag C/2025 J1 (Borisov)
13:34:03.03 +46:12:46.9 15.2mag C/2025 L1 (ATLAS)
03:27:06.90 -26:23:37.7 17.8mag C/2025 Q3 (ATLAS)
23:54:33.38 +18:09:01.6 8.3mag C/2025 R3 (PANSTARRS)
12:53:37.20 +03:04:56.3 17.4mag C/2025 Y1 (ATLAS)
03:37:02.05 +02:30:15.0 13.6mag C/2026 A1 (MAPS)
00:02:50.23 +37:25:43.6 14.6mag C/2026 B2 (Sun-Gao)
18:45:11.10 -09:39:24.3 11.8mag 10P/Tempel
14:58:44.19 +03:05:10.8 14.1mag 24P/Schaumasse
11:02:30.12 -01:29:22.2 15.7mag 29P/Schwassmann-Wachmann
18:01:16.05 -09:34:06.0 18.0mag 40P/Vaisala
10:37:32.29 -04:00:32.1 16.9mag 43P/Wolf-Harrington
01:50:27.82 +17:41:02.6 17.2mag 47P/Ashbrook-Jackson
07:12:54.66 +36:45:48.8 17.0mag 63P/Wild
23:30:31.52 -11:18:45.6 15.7mag 65P/Gunn
04:06:21.14 +21:38:55.4 15.9mag 76P/West-Kohoutek-Ikemura
01:08:08.10 +08:27:19.1 14.3mag 78P/Gehrels
23:06:29.16 -09:02:56.6 14.6mag 88P/Howell
02:13:41.04 +20:56:53.9 15.1mag 93P/Lovas
04:56:59.76 +32:20:54.5 16.2mag 123P/West-Hartley
08:29:44.74 +37:49:41.8 16.2mag 124P/Mrkos
02:35:00.33 +14:29:54.2 16.4mag 128P/Shoemaker-Holt
02:49:48.44 +14:37:59.0 17.5mag 131P/Mueller
01:32:15.82 +13:37:51.8 10.6mag 141P/Machholz
01:41:01.43 +05:18:23.7 10.6mag 141P-A/Machholz
00:25:46.82 +01:10:37.2 12.7mag 141P-D/Machholz
02:11:26.26 +07:03:58.6 17.8mag 141P-I/Machholz
01:05:36.38 -00:56:36.4 15.1mag 162P/SidingSpring
14:49:23.06 +00:02:52.8 17.7mag 210P/Christensen
21:42:09.34 -11:10:14.1 17.6mag 218P/LINEAR
17:16:49.47 -13:47:36.7 16.1mag 235P/LINEAR
05:36:59.17 +34:47:02.9 16.8mag 240P/NEAT
07:39:04.41 -05:02:36.7 17.7mag 242P/Spahr
22:19:47.93 -20:40:09.9 17.9mag 260P/McNaught
02:00:33.28 +20:45:01.6 18.0mag 295P/LINEAR
15:42:11.13 +07:03:56.4 17.5mag 391P/Kowalski
07:34:39.05 +21:22:08.6 17.7mag 450P/LONEOS
05:37:33.91 +44:57:54.6 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 16 22:53 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
17:21:59.44 -38:54:04.60 2026-04-14.4 15.15
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
-rw-r--r-- 1 apache apache 5.8K Apr 16 22:53 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 16 22:53 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:06:56.603 -64:55:52.46 AT 2026jcy 2026-04-09.11 18.906
08:27:06.222 -58:50:26.83 AT 2026jcx 2026-04-09.08 19.372
13:48:22.893 -31:10:42.12 AT 2026jcw 2026-04-09.08 19.95
17:39:28.750 +05:01:10.80 AT 2026jcv 2026-04-09.86 16.87
14:44:31.580 +71:55:25.90 AT 2026jcu 2026-04-09.47 17.9
12:39:27.288 -08:14:32.64 AT 2026jct 2026-04-09.53 20.16
14:15:21.948 -35:02:48.79 AT 2026jcs 2026-04-09.59 19.67
12:55:53.000 +08:04:22.00 AT 2026jcr 2026-04-09.62 22.1051
12:29:42.630 -28:00:38.18 AT 2026jcq 2026-04-09.56 18.99
13:00:14.826 -06:35:50.60 AT 2026jcp 2026-04-09.56 19.7
12:54:45.376 +09:10:41.41 AT 2026jco 2026-04-09.62 20.9256
13:25:12.570 -33:30:18.80 AT 2026jcn 2026-04-07.60 19.74
13:20:52.501 -35:57:03.67 AT 2026jcm 2026-04-07.60 20.01
12:07:08.367 +13:12:39.86 AT 2026jcl 2026-04-09.62 22.8073
12:11:43.063 +14:00:46.62 AT 2026jck 2026-04-09.62 21.8834
14:57:35.040 -17:11:22.89 AT 2026jcj 2026-04-09.58 19.52
15:09:26.181 -10:41:27.18 AT 2026jci 2026-04-09.45 20.2
18:22:34.467 +53:35:59.16 AT 2026jch 2026-04-05.40 19.7444
15:13:25.280 +39:43:46.60 AT 2026jcg 2026-03-30.81 21.1
17:32:02.830 +27:34:31.03 AT 2026jcf 2026-03-27.92 21.46
-rw-r--r-- 1 apache apache 30K Apr 16 22:53 tns_transients_list.txt
